lidar_correction_ghk.py

Tue, 15 Nov 2016 03:44:26 +0100

author
Volker Freudenthaler <volker.freudenthaler@lmu.de>
date
Tue, 15 Nov 2016 03:44:26 +0100
changeset 14
82dba9904149
parent 13
f08818615e3a
child 16
313ac320b970
permissions
-rw-r--r--

update

ulalume3@0 1 # -*- coding: utf-8 -*-
ulalume3@0 2 """
ulalume3@0 3 Copyright 2016 Volker Freudenthaler
ulalume3@0 4
ulalume3@0 5 Licensed under the EUPL, Version 1.1 only (the "Licence").
ulalume3@0 6
ulalume3@0 7 You may not use this work except in compliance with the Licence.
ulalume3@0 8 A copy of the licence is distributed with the code. Alternatively, you may obtain
ulalume3@0 9 a copy of the Licence at:
ulalume3@0 10
ulalume3@0 11 https://joinup.ec.europa.eu/community/eupl/og_page/eupl
ulalume3@0 12
ulalume3@0 13 Unless required by applicable law or agreed to in writing, software distributed
ulalume3@0 14 under the Licence is distributed on an "AS IS" basis, WITHOUT WARRANTIES OR CONDITIONS
ulalume3@0 15 OF ANY KIND, either express or implied. See the Licence for the specific language governing
ulalume3@0 16 permissions and limitations under the Licence.
ulalume3@0 17
ulalume3@0 18 Equation reference: http://www.atmos-meas-tech-discuss.net/amt-2015-338/amt-2015-338.pdf
ulalume3@0 19 With equations code from Appendix C
volker@11 20 Python 3.4.2
ulalume3@0 21 """
ulalume3@0 22 #!/usr/bin/env python3
volker@11 23
volker@11 24 # Comment: The code works with Python 2.7 with the help of following line, which enables Python2 to correctly interpret the Python 3 print statements.
ulalume3@0 25 from __future__ import print_function
ulalume3@0 26 #import math
ulalume3@0 27 import numpy as np
ulalume3@0 28 import sys
ulalume3@0 29 import os
ulalume3@0 30
volker@11 31 # Comment: the seaborn library makes nicer plots, but the code works also without it.
volker@11 32 try:
volker@11 33 import seaborn as sns
volker@11 34 sns_loaded = True
volker@11 35 except ImportError:
volker@11 36 sns_loaded = False
volker@11 37
ulalume3@0 38 import matplotlib.pyplot as plt
ulalume3@0 39 from time import clock
ulalume3@0 40
ulalume3@0 41 #from matplotlib.backends.backend_pdf import PdfPages
ulalume3@0 42 #pdffile = '{}.pdf'.format('path')
ulalume3@0 43 #pp = PdfPages(pdffile)
ulalume3@0 44 ## pp.savefig can be called multiple times to save to multiple pages
ulalume3@0 45 #pp.savefig()
ulalume3@0 46 #pp.close()
ulalume3@0 47
ulalume3@0 48 from contextlib import contextmanager
ulalume3@0 49 @contextmanager
ulalume3@0 50 def redirect_stdout(new_target):
ulalume3@0 51 old_target, sys.stdout = sys.stdout, new_target # replace sys.stdout
ulalume3@0 52 try:
ulalume3@0 53 yield new_target # run some code with the replaced stdout
ulalume3@0 54 finally:
ulalume3@0 55 sys.stdout.flush()
ulalume3@0 56 sys.stdout = old_target # restore to the previous value
ulalume3@0 57 '''
ulalume3@0 58 real_raw_input = vars(__builtins__).get('raw_input',input)
ulalume3@0 59 '''
ulalume3@0 60 try:
ulalume3@0 61 import __builtin__
ulalume3@0 62 input = getattr(__builtin__, 'raw_input')
ulalume3@0 63 except (ImportError, AttributeError):
ulalume3@0 64 pass
ulalume3@0 65
ulalume3@0 66 from distutils.util import strtobool
ulalume3@0 67 def user_yes_no_query(question):
ulalume3@0 68 sys.stdout.write('%s [y/n]\n' % question)
ulalume3@0 69 while True:
ulalume3@0 70 try:
ulalume3@0 71 return strtobool(input().lower())
ulalume3@0 72 except ValueError:
ulalume3@0 73 sys.stdout.write('Please respond with \'y\' or \'n\'.\n')
ulalume3@0 74
ulalume3@0 75 #if user_yes_no_query('want to exit?') == 1: sys.exit()
ulalume3@0 76
ulalume3@0 77 abspath = os.path.abspath(__file__)
ulalume3@0 78 dname = os.path.dirname(abspath)
ulalume3@0 79 fname = os.path.basename(abspath)
ulalume3@0 80 os.chdir(dname)
ulalume3@0 81
ulalume3@0 82 #PrintToOutputFile = True
ulalume3@0 83
ulalume3@0 84 sqr05 = 0.5**0.5
ulalume3@0 85
ulalume3@0 86 # ---- Initial definition of variables; the actual values will be read in with exec(open('./optic_input.py').read()) below
ulalume3@0 87 LID = "internal"
ulalume3@0 88 EID = "internal"
ulalume3@0 89 # --- IL Laser IL and +-Uncertainty
ulalume3@0 90 bL = 1. #degree of linear polarization; default 1
ulalume3@0 91 RotL, dRotL, nRotL = 0.0, 0.0, 1 #alpha; rotation of laser polarization in degrees; default 0
ulalume3@0 92 # --- ME Emitter and +-Uncertainty
ulalume3@0 93 DiE, dDiE, nDiE = 0., 0.00, 1 # Diattenuation
ulalume3@0 94 TiE = 1. # Unpolarized transmittance
ulalume3@0 95 RetE, dRetE, nRetE = 0., 180.0, 0 # Retardance in degrees
ulalume3@0 96 RotE, dRotE, nRotE = 0., 0.0, 0 # beta: Rotation of optical element in degrees
ulalume3@0 97 # --- MO Receiver Optics including telescope
ulalume3@0 98 DiO, dDiO, nDiO = -0.055, 0.003, 1
ulalume3@0 99 TiO = 0.9
ulalume3@0 100 RetO, dRetO, nRetO = 0., 180.0, 2
ulalume3@0 101 RotO, dRotO, nRotO = 0., 0.1, 1 #gamma
ulalume3@0 102 # --- PBS MT transmitting path defined with (TS,TP); and +-Uncertainty
ulalume3@0 103 TP, dTP, nTP = 0.98, 0.02, 1
ulalume3@0 104 TS, dTS, nTS = 0.001, 0.001, 1
ulalume3@0 105 TiT = 0.5 * (TP + TS)
ulalume3@0 106 DiT = (TP-TS)/(TP+TS)
ulalume3@0 107 # PolFilter
ulalume3@0 108 RetT, dRetT, nRetT = 0., 180., 0
ulalume3@0 109 ERaT, dERaT, nERaT = 0.001, 0.001, 1
ulalume3@0 110 RotaT, dRotaT, nRotaT = 0., 3., 1
ulalume3@0 111 DaT = (1-ERaT)/(1+ERaT)
ulalume3@0 112 TaT = 0.5*(1+ERaT)
ulalume3@0 113 # --- PBS MR reflecting path defined with (RS,RP); and +-Uncertainty
volker@13 114 RS_RP_depend_on_TS_TP = False
volker@13 115 if(RS_RP_depend_on_TS_TP):
volker@13 116 RP, dRP, nRP = 1-TP, 0.00, 0
volker@13 117 RS, dRS, nRS = 1-TS, 0.00, 0
volker@13 118 else:
volker@13 119 RP, dRP, nRP = 0.05, 0.01, 1
volker@13 120 RS, dRS, nRS = 0.98, 0.01, 1
ulalume3@0 121 TiR = 0.5 * (RP + RS)
ulalume3@0 122 DiR = (RP-RS)/(RP+RS)
ulalume3@0 123 # PolFilter
ulalume3@0 124 RetR, dRetR, nRetR = 0., 180., 0
ulalume3@0 125 ERaR, dERaR, nERaR = 0.001, 0.001, 1
ulalume3@0 126 RotaR,dRotaR,nRotaR = 90., 3., 1
ulalume3@0 127 DaR = (1-ERaR)/(1+ERaR)
ulalume3@0 128 TaR = 0.5*(1+ERaR)
ulalume3@0 129
ulalume3@0 130 # Parellel signal detected in the transmitted channel => Y = 1, or in the reflected channel => Y = -1
ulalume3@0 131 Y = -1.
ulalume3@0 132
ulalume3@0 133 # Calibrator = type defined by matrix values
ulalume3@0 134 LocC = 4 # location of calibrator: behind laser = 1; behind emitter = 2; before receiver = 3; before PBS = 4
ulalume3@0 135
ulalume3@0 136 TypeC = 3 # linear polarizer calibrator
ulalume3@0 137 # example with extinction ratio 0.001
ulalume3@0 138 DiC, dDiC, nDiC = 1.0, 0., 0 # ideal 1.0
ulalume3@0 139 TiC = 0.5 # ideal 0.5
ulalume3@0 140 RetC, dRetC, nRetC = 0., 0., 0
ulalume3@0 141 RotC, dRotC, nRotC = 0.0, 0.1, 0 #constant calibrator offset epsilon
ulalume3@0 142 RotationErrorEpsilonForNormalMeasurements = False # is in general False for TypeC == 3 calibrator
ulalume3@0 143
ulalume3@0 144 # Rotation error without calibrator: if False, then epsilon = 0 for normal measurements
ulalume3@0 145 RotationErrorEpsilonForNormalMeasurements = True
ulalume3@0 146
ulalume3@0 147 # LDRCal assumed atmospheric linear depolarization ratio during the calibration measurements (first guess)
ulalume3@0 148 LDRCal0,dLDRCal,nLDRCal= 0.25, 0.04, 1
ulalume3@0 149 LDRCal = LDRCal0
ulalume3@0 150 # measured LDRm will be corrected with calculated parameters
ulalume3@0 151 LDRmeas = 0.015
ulalume3@0 152 # LDRtrue for simulation of measurement => LDRsim
ulalume3@0 153 LDRtrue = 0.5
ulalume3@0 154 LDRtrue2 = 0.004
ulalume3@0 155
ulalume3@0 156 # Initialize other values to 0
ulalume3@0 157 ER, nER, dER = 0.001, 0, 0.001
ulalume3@0 158 K = 0.
ulalume3@0 159 Km = 0.
ulalume3@0 160 Kp = 0.
ulalume3@0 161 LDRcorr = 0.
ulalume3@0 162 Eta = 0.
ulalume3@0 163 Ir = 0.
ulalume3@0 164 It = 0.
ulalume3@0 165 h = 1.
ulalume3@0 166
ulalume3@0 167 Loc = ['', 'behind laser', 'behind emitter', 'before receiver', 'before PBS']
ulalume3@0 168 Type = ['', 'mechanical rotator', 'hwp rotator', 'linear polarizer', 'qwp rotator', 'circular polarizer', 'real HWP +-22.5°']
ulalume3@0 169 dY = ['reflected channel', '', 'transmitted channel']
ulalume3@0 170
ulalume3@0 171 # end of initial definition of variables
ulalume3@0 172 # *******************************************************************************************************************************
ulalume3@0 173
ulalume3@0 174 # --- Read actual lidar system parameters from ./optic_input.py (must be in the same directory)
ulalume3@0 175
volker@11 176 InputFile = 'optic_input_example_lidar.py'
ulalume3@0 177 #InputFile = 'optic_input_ver6e_POLIS_355.py'
ulalume3@0 178 #InputFile = 'optic_input_ver6e_POLIS_355_JA.py'
ulalume3@0 179 #InputFile = 'optic_input_ver6c_POLIS_532.py'
ulalume3@0 180 #InputFile = 'optic_input_ver6e_POLIS_532.py'
ulalume3@0 181 #InputFile = 'optic_input_ver8c_POLIS_532.py'
ulalume3@0 182 #InputFile = 'optic_input_ver6e_MUSA.py'
ulalume3@0 183 #InputFile = 'optic_input_ver6e_MUSA_JA.py'
ulalume3@0 184 #InputFile = 'optic_input_ver6e_PollyXTSea.py'
ulalume3@0 185 #InputFile = 'optic_input_ver6e_PollyXTSea_JA.py'
ulalume3@0 186 #InputFile = 'optic_input_ver6e_PollyXT_RALPH.py'
ulalume3@0 187 #InputFile = 'optic_input_ver8c_PollyXT_RALPH.py'
ulalume3@0 188 #InputFile = 'optic_input_ver8c_PollyXT_RALPH_2.py'
ulalume3@0 189 #InputFile = 'optic_input_ver8c_PollyXT_RALPH_3.py'
ulalume3@0 190 #InputFile = 'optic_input_ver8c_PollyXT_RALPH_4.py'
ulalume3@0 191 #InputFile = 'optic_input_ver8c_PollyXT_RALPH_5.py'
ulalume3@0 192 #InputFile = 'optic_input_ver8c_PollyXT_RALPH_6.py'
volker@11 193 #InputFile = 'optic_input_ver8c_PollyXT_RALPH_7.py'
ulalume3@0 194 #InputFile = 'optic_input_ver8a_MOHP_DPL_355.py'
ulalume3@0 195 #InputFile = 'optic_input_ver9_MOHP_DPL_355.py'
ulalume3@0 196 #InputFile = 'optic_input_ver6e_RALI.py'
ulalume3@0 197 #InputFile = 'optic_input_ver6e_RALI_JA.py'
ulalume3@0 198 #InputFile = 'optic_input_ver6e_RALI_new.py'
ulalume3@0 199 #InputFile = 'optic_input_ver6e_RALI_act.py'
ulalume3@0 200 #InputFile = 'optic_input_ver6e_MULHACEN.py'
ulalume3@0 201 #InputFile = 'optic_input_ver6e_MULHACEN_JA.py'
ulalume3@0 202 #InputFile = 'optic_input_ver6e-IPRAL.py'
ulalume3@0 203 #InputFile = 'optic_input_ver6e-IPRAL_JA.py'
ulalume3@0 204 #InputFile = 'optic_input_ver6e-LB21.py'
ulalume3@0 205 #InputFile = 'optic_input_ver6e-LB21_JA.py'
ulalume3@0 206 #InputFile = 'optic_input_ver6e_Bertha_b_355.py'
ulalume3@0 207 #InputFile = 'optic_input_ver6e_Bertha_b_532.py'
ulalume3@0 208 #InputFile = 'optic_input_ver6e_Bertha_b_1064.py'
ulalume3@0 209
ulalume3@0 210 '''
ulalume3@0 211 print("From ", dname)
ulalume3@0 212 print("Running ", fname)
ulalume3@0 213 print("Reading input file ", InputFile, " for")
ulalume3@0 214 '''
ulalume3@0 215 input_path = os.path.join('.', 'system_settings', InputFile)
ulalume3@0 216 # this works with Python 2 - and 3?
ulalume3@0 217 exec(open(input_path).read(), globals())
ulalume3@0 218 # end of read actual system parameters
ulalume3@0 219
ulalume3@0 220 # --- Manual Parameter Change ---
ulalume3@0 221 # (use for quick parameter changes without changing the input file )
ulalume3@0 222 #DiO = 0.
ulalume3@0 223 #LDRtrue = 0.45
ulalume3@0 224 #LDRtrue2 = 0.004
ulalume3@0 225 #Y = -1
ulalume3@0 226 #LocC = 4 #location of calibrator: 1 = behind laser; 2 = behind emitter; 3 = before receiver; 4 = before PBS
ulalume3@0 227 ##TypeC = 6 Don't change the TypeC here
ulalume3@0 228 #RotationErrorEpsilonForNormalMeasurements = True
ulalume3@0 229 #LDRCal = 0.25
ulalume3@0 230 #bL = 0.8
ulalume3@0 231 ## --- Errors
ulalume3@0 232 RotL0, dRotL, nRotL = RotL, dRotL, nRotL
ulalume3@0 233
ulalume3@0 234 DiE0, dDiE, nDiE = DiE, dDiE, nDiE
ulalume3@0 235 RetE0, dRetE, nRetE = RetE, dRetE, nRetE
ulalume3@0 236 RotE0, dRotE, nRotE = RotE, dRotE, nRotE
ulalume3@0 237
ulalume3@0 238 DiO0, dDiO, nDiO = DiO, dDiO, nDiO
ulalume3@0 239 RetO0, dRetO, nRetO = RetO, dRetO, nRetO
ulalume3@0 240 RotO0, dRotO, nRotO = RotO, dRotO, nRotO
ulalume3@0 241
ulalume3@0 242 DiC0, dDiC, nDiC = DiC, dDiC, nDiC
ulalume3@0 243 RetC0, dRetC, nRetC = RetC, dRetC, nRetC
ulalume3@0 244 RotC0, dRotC, nRotC = RotC, dRotC, nRotC
ulalume3@0 245
ulalume3@0 246 TP0, dTP, nTP = TP, dTP, nTP
ulalume3@0 247 TS0, dTS, nTS = TS, dTS, nTS
ulalume3@0 248 RetT0, dRetT, nRetT = RetT, dRetT, nRetT
ulalume3@0 249
ulalume3@0 250 ERaT0, dERaT, nERaT = ERaT, dERaT, nERaT
ulalume3@0 251 RotaT0,dRotaT,nRotaT= RotaT,dRotaT,nRotaT
ulalume3@0 252
ulalume3@0 253 RP0, dRP, nRP = RP, dRP, nRP
ulalume3@0 254 RS0, dRS, nRS = RS, dRS, nRS
ulalume3@0 255 RetR0, dRetR, nRetR = RetR, dRetR, nRetR
ulalume3@0 256
ulalume3@0 257 ERaR0, dERaR, nERaR = ERaR, dERaR, nERaR
ulalume3@0 258 RotaR0,dRotaR,nRotaR= RotaR,dRotaR,nRotaR
ulalume3@0 259
ulalume3@0 260 LDRCal0,dLDRCal,nLDRCal=LDRCal,dLDRCal,nLDRCal
ulalume3@0 261 #LDRCal0,dLDRCal,nLDRCal=LDRCal,dLDRCal,0
ulalume3@0 262 # ---------- End of manual parameter change
ulalume3@0 263
ulalume3@0 264 RotL, RotE, RetE, DiE, RotO, RetO, DiO, RotC, RetC, DiC = RotL0, RotE0, RetE0, DiE0, RotO0, RetO0, DiO0, RotC0, RetC0, DiC0
ulalume3@0 265 TP, TS, RP, RS, ERaT, RotaT, RetT, ERaR, RotaR, RetR = TP0, TS0, RP0, RS0 , ERaT0, RotaT0, RetT0, ERaR0, RotaR0, RetR0
ulalume3@0 266 LDRCal = LDRCal0
ulalume3@0 267 DTa0, TTa0, DRa0, TRa0, LDRsimx, LDRCorr = 0,0,0,0,0,0
ulalume3@0 268
ulalume3@0 269 TiT = 0.5 * (TP + TS)
ulalume3@0 270 DiT = (TP-TS)/(TP+TS)
ulalume3@0 271 ZiT = (1. - DiT**2)**0.5
ulalume3@0 272 TiR = 0.5 * (RP + RS)
ulalume3@0 273 DiR = (RP-RS)/(RP+RS)
ulalume3@0 274 ZiR = (1. - DiR**2)**0.5
ulalume3@0 275
volker@13 276 # --- this subroutine is for the calculation with certain fixed parameters -----------------------------------------------------
ulalume3@0 277 def Calc(RotL, RotE, RetE, DiE, RotO, RetO, DiO, RotC, RetC, DiC, TP, TS, RP, RS, ERaT, RotaT, RetT, ERaR, RotaR, RetR, LDRCal):
ulalume3@0 278 # ---- Do the calculations of bra-ket vectors
ulalume3@0 279 h = -1. if TypeC == 2 else 1
ulalume3@0 280 # from input file: assumed LDRCal for calibration measurements
ulalume3@0 281 aCal = (1.-LDRCal)/(1+LDRCal)
ulalume3@0 282 # from input file: measured LDRm and true LDRtrue, LDRtrue2 =>
ulalume3@0 283 #ameas = (1.-LDRmeas)/(1+LDRmeas)
ulalume3@0 284 atrue = (1.-LDRtrue)/(1+LDRtrue)
ulalume3@0 285 #atrue2 = (1.-LDRtrue2)/(1+LDRtrue2)
ulalume3@0 286
ulalume3@0 287 # angles of emitter and laser and calibrator and receiver optics
ulalume3@0 288 # RotL = alpha, RotE = beta, RotO = gamma, RotC = epsilon
ulalume3@0 289 S2a = np.sin(2*np.deg2rad(RotL))
ulalume3@0 290 C2a = np.cos(2*np.deg2rad(RotL))
ulalume3@0 291 S2b = np.sin(2*np.deg2rad(RotE))
ulalume3@0 292 C2b = np.cos(2*np.deg2rad(RotE))
ulalume3@0 293 S2ab = np.sin(np.deg2rad(2*RotL-2*RotE))
ulalume3@0 294 C2ab = np.cos(np.deg2rad(2*RotL-2*RotE))
ulalume3@0 295 S2g = np.sin(np.deg2rad(2*RotO))
ulalume3@0 296 C2g = np.cos(np.deg2rad(2*RotO))
ulalume3@0 297
ulalume3@0 298 # Laser with Degree of linear polarization DOLP = bL
ulalume3@0 299 IinL = 1.
ulalume3@0 300 QinL = bL
ulalume3@0 301 UinL = 0.
ulalume3@0 302 VinL = (1. - bL**2)**0.5
ulalume3@0 303
ulalume3@0 304 # Stokes Input Vector rotation Eq. E.4
ulalume3@0 305 A = C2a*QinL - S2a*UinL
ulalume3@0 306 B = S2a*QinL + C2a*UinL
ulalume3@0 307 # Stokes Input Vector rotation Eq. E.9
ulalume3@0 308 C = C2ab*QinL - S2ab*UinL
ulalume3@0 309 D = S2ab*QinL + C2ab*UinL
ulalume3@0 310
ulalume3@0 311 # emitter optics
ulalume3@0 312 CosE = np.cos(np.deg2rad(RetE))
ulalume3@0 313 SinE = np.sin(np.deg2rad(RetE))
ulalume3@0 314 ZiE = (1. - DiE**2)**0.5
ulalume3@0 315 WiE = (1. - ZiE*CosE)
ulalume3@0 316
ulalume3@0 317 # Stokes Input Vector after emitter optics equivalent to Eq. E.9 with already rotated input vector from Eq. E.4
ulalume3@0 318 # b = beta
ulalume3@0 319 IinE = (IinL + DiE*C)
ulalume3@0 320 QinE = (C2b*DiE*IinL + A + S2b*(WiE*D - ZiE*SinE*VinL))
ulalume3@0 321 UinE = (S2b*DiE*IinL + B - C2b*(WiE*D - ZiE*SinE*VinL))
ulalume3@0 322 VinE = (-ZiE*SinE*D + ZiE*CosE*VinL)
ulalume3@0 323
ulalume3@0 324 # Stokes Input Vector before receiver optics Eq. E.19 (after atmosphere F)
ulalume3@0 325 IinF = IinE
ulalume3@0 326 QinF = aCal*QinE
ulalume3@0 327 UinF = -aCal*UinE
ulalume3@0 328 VinF = (1.-2.*aCal)*VinE
ulalume3@0 329
ulalume3@0 330 # receiver optics
ulalume3@0 331 CosO = np.cos(np.deg2rad(RetO))
ulalume3@0 332 SinO = np.sin(np.deg2rad(RetO))
ulalume3@0 333 ZiO = (1. - DiO**2)**0.5
ulalume3@0 334 WiO = (1. - ZiO*CosO)
ulalume3@0 335
ulalume3@0 336 # calibrator
ulalume3@0 337 CosC = np.cos(np.deg2rad(RetC))
ulalume3@0 338 SinC = np.sin(np.deg2rad(RetC))
ulalume3@0 339 ZiC = (1. - DiC**2)**0.5
ulalume3@0 340 WiC = (1. - ZiC*CosC)
ulalume3@0 341
ulalume3@0 342 # Stokes Input Vector before the polarising beam splitter Eq. E.31
ulalume3@0 343 A = C2g*QinE - S2g*UinE
ulalume3@0 344 B = S2g*QinE + C2g*UinE
ulalume3@0 345
ulalume3@0 346 IinP = (IinE + DiO*aCal*A)
ulalume3@0 347 QinP = (C2g*DiO*IinE + aCal*QinE - S2g*(WiO*aCal*B + ZiO*SinO*(1-2*aCal)*VinE))
ulalume3@0 348 UinP = (S2g*DiO*IinE - aCal*UinE + C2g*(WiO*aCal*B + ZiO*SinO*(1-2*aCal)*VinE))
ulalume3@0 349 VinP = (ZiO*SinO*aCal*B + ZiO*CosO*(1-2*aCal)*VinE)
ulalume3@0 350
ulalume3@0 351 #-------------------------
ulalume3@0 352 # F11 assuemd to be = 1 => measured: F11m = IinP / IinE with atrue
ulalume3@0 353 #F11sim = TiO*(IinE + DiO*atrue*A)/IinE
ulalume3@0 354 #-------------------------
ulalume3@0 355
ulalume3@0 356 # analyser
volker@13 357 #For POLLY_XTs
volker@13 358 if(RS_RP_depend_on_TS_TP):
volker@13 359 RS = 1 - TS
volker@13 360 RP = 1 - TP
ulalume3@0 361 TiT = 0.5 * (TP + TS)
ulalume3@0 362 DiT = (TP-TS)/(TP+TS)
ulalume3@0 363 ZiT = (1. - DiT**2)**0.5
ulalume3@0 364 TiR = 0.5 * (RP + RS)
ulalume3@0 365 DiR = (RP-RS)/(RP+RS)
ulalume3@0 366 ZiR = (1. - DiR**2)**0.5
ulalume3@0 367 CosT = np.cos(np.deg2rad(RetT))
ulalume3@0 368 SinT = np.sin(np.deg2rad(RetT))
ulalume3@0 369 CosR = np.cos(np.deg2rad(RetR))
ulalume3@0 370 SinR = np.sin(np.deg2rad(RetR))
ulalume3@0 371
ulalume3@0 372 DaT = (1-ERaT)/(1+ERaT)
ulalume3@0 373 DaR = (1-ERaR)/(1+ERaR)
ulalume3@0 374 TaT = 0.5*(1+ERaT)
ulalume3@0 375 TaR = 0.5*(1+ERaR)
ulalume3@0 376
ulalume3@0 377 S2aT = np.sin(np.deg2rad(h*2*RotaT))
ulalume3@0 378 C2aT = np.cos(np.deg2rad(2*RotaT))
ulalume3@0 379 S2aR = np.sin(np.deg2rad(h*2*RotaR))
ulalume3@0 380 C2aR = np.cos(np.deg2rad(2*RotaR))
ulalume3@0 381
ulalume3@0 382 # Aanalyzer As before the PBS Eq. D.5
ulalume3@0 383 ATP1 = (1+C2aT*DaT*DiT)
ulalume3@0 384 ATP2 = Y*(DiT+C2aT*DaT)
ulalume3@0 385 ATP3 = Y*S2aT*DaT*ZiT*CosT
ulalume3@0 386 ATP4 = S2aT*DaT*ZiT*SinT
ulalume3@0 387 ATP = np.array([ATP1,ATP2,ATP3,ATP4])
ulalume3@0 388
ulalume3@0 389 ARP1 = (1+C2aR*DaR*DiR)
ulalume3@0 390 ARP2 = Y*(DiR+C2aR*DaR)
ulalume3@0 391 ARP3 = Y*S2aR*DaR*ZiR*CosR
ulalume3@0 392 ARP4 = S2aR*DaR*ZiR*SinR
ulalume3@0 393 ARP = np.array([ARP1,ARP2,ARP3,ARP4])
ulalume3@0 394
ulalume3@0 395 DTa = ATP2*Y/ATP1
ulalume3@0 396 DRa = ARP2*Y/ARP1
ulalume3@0 397
ulalume3@0 398 # ---- Calculate signals and correction parameters for diffeent locations and calibrators
ulalume3@0 399 if LocC == 4: # Calibrator before the PBS
ulalume3@0 400 #print("Calibrator location not implemented yet")
ulalume3@0 401
ulalume3@0 402 #S2ge = np.sin(np.deg2rad(2*RotO + h*2*RotC))
ulalume3@0 403 #C2ge = np.cos(np.deg2rad(2*RotO + h*2*RotC))
ulalume3@0 404 S2e = np.sin(np.deg2rad(h*2*RotC))
ulalume3@0 405 C2e = np.cos(np.deg2rad(2*RotC))
ulalume3@0 406 # rotated AinP by epsilon Eq. C.3
ulalume3@0 407 ATP2e = C2e*ATP2 + S2e*ATP3
ulalume3@0 408 ATP3e = C2e*ATP3 - S2e*ATP2
ulalume3@0 409 ARP2e = C2e*ARP2 + S2e*ARP3
ulalume3@0 410 ARP3e = C2e*ARP3 - S2e*ARP2
ulalume3@0 411 ATPe = np.array([ATP1,ATP2e,ATP3e,ATP4])
ulalume3@0 412 ARPe = np.array([ARP1,ARP2e,ARP3e,ARP4])
ulalume3@0 413 # Stokes Input Vector before the polarising beam splitter Eq. E.31
ulalume3@0 414 A = C2g*QinE - S2g*UinE
ulalume3@0 415 B = S2g*QinE + C2g*UinE
ulalume3@0 416 #C = (WiO*aCal*B + ZiO*SinO*(1-2*aCal)*VinE)
ulalume3@0 417 Co = ZiO*SinO*VinE
ulalume3@0 418 Ca = (WiO*B - 2*ZiO*SinO*VinE)
ulalume3@0 419 #C = Co + aCal*Ca
ulalume3@0 420 #IinP = (IinE + DiO*aCal*A)
ulalume3@0 421 #QinP = (C2g*DiO*IinE + aCal*QinE - S2g*C)
ulalume3@0 422 #UinP = (S2g*DiO*IinE - aCal*UinE + C2g*C)
ulalume3@0 423 #VinP = (ZiO*SinO*aCal*B + ZiO*CosO*(1-2*aCal)*VinE)
ulalume3@0 424 IinPo = IinE
ulalume3@0 425 QinPo = (C2g*DiO*IinE - S2g*Co)
ulalume3@0 426 UinPo = (S2g*DiO*IinE + C2g*Co)
ulalume3@0 427 VinPo = ZiO*CosO*VinE
ulalume3@0 428
ulalume3@0 429 IinPa = DiO*A
ulalume3@0 430 QinPa = QinE - S2g*Ca
ulalume3@0 431 UinPa = -UinE + C2g*Ca
ulalume3@0 432 VinPa = ZiO*(SinO*B - 2*CosO*VinE)
ulalume3@0 433
ulalume3@0 434 IinP = IinPo + aCal*IinPa
ulalume3@0 435 QinP = QinPo + aCal*QinPa
ulalume3@0 436 UinP = UinPo + aCal*UinPa
ulalume3@0 437 VinP = VinPo + aCal*VinPa
ulalume3@0 438 # Stokes Input Vector before the polarising beam splitter rotated by epsilon Eq. C.3
ulalume3@0 439 #QinPe = C2e*QinP + S2e*UinP
ulalume3@0 440 #UinPe = C2e*UinP - S2e*QinP
ulalume3@0 441 QinPoe = C2e*QinPo + S2e*UinPo
ulalume3@0 442 UinPoe = C2e*UinPo - S2e*QinPo
ulalume3@0 443 QinPae = C2e*QinPa + S2e*UinPa
ulalume3@0 444 UinPae = C2e*UinPa - S2e*QinPa
ulalume3@0 445 QinPe = C2e*QinP + S2e*UinP
ulalume3@0 446 UinPe = C2e*UinP - S2e*QinP
ulalume3@0 447
ulalume3@0 448 # Calibration signals and Calibration correction K from measurements with LDRCal / aCal
ulalume3@0 449 if (TypeC == 2) or (TypeC == 1): # rotator calibration Eq. C.4
ulalume3@0 450 # parameters for calibration with aCal
ulalume3@0 451 AT = ATP1*IinP + h*ATP4*VinP
ulalume3@0 452 BT = ATP3e*QinP - h*ATP2e*UinP
ulalume3@0 453 AR = ARP1*IinP + h*ARP4*VinP
ulalume3@0 454 BR = ARP3e*QinP - h*ARP2e*UinP
ulalume3@0 455 # Correction paremeters for normal measurements; they are independent of LDR
ulalume3@0 456 if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out
ulalume3@0 457 IS1 = np.array([IinPo,QinPo,UinPo,VinPo])
ulalume3@0 458 IS2 = np.array([IinPa,QinPa,UinPa,VinPa])
ulalume3@0 459 GT = np.dot(ATP,IS1)
ulalume3@0 460 GR = np.dot(ARP,IS1)
ulalume3@0 461 HT = np.dot(ATP,IS2)
ulalume3@0 462 HR = np.dot(ARP,IS2)
ulalume3@0 463 else:
ulalume3@0 464 IS1 = np.array([IinPo,QinPo,UinPo,VinPo])
ulalume3@0 465 IS2 = np.array([IinPa,QinPa,UinPa,VinPa])
ulalume3@0 466 GT = np.dot(ATPe,IS1)
ulalume3@0 467 GR = np.dot(ARPe,IS1)
ulalume3@0 468 HT = np.dot(ATPe,IS2)
ulalume3@0 469 HR = np.dot(ARPe,IS2)
ulalume3@0 470 elif (TypeC == 3) or (TypeC == 4): # linear polariser calibration Eq. C.5
ulalume3@0 471 # parameters for calibration with aCal
ulalume3@0 472 AT = ATP1*IinP + ATP3e*UinPe + ZiC*CosC*(ATP2e*QinPe + ATP4*VinP)
ulalume3@0 473 BT = DiC*(ATP1*UinPe + ATP3e*IinP) - ZiC*SinC*(ATP2e*VinP - ATP4*QinPe)
ulalume3@0 474 AR = ARP1*IinP + ARP3e*UinPe + ZiC*CosC*(ARP2e*QinPe + ARP4*VinP)
ulalume3@0 475 BR = DiC*(ARP1*UinPe + ARP3e*IinP) - ZiC*SinC*(ARP2e*VinP - ARP4*QinPe)
ulalume3@0 476 # Correction paremeters for normal measurements; they are independent of LDR
ulalume3@0 477 if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out
ulalume3@0 478 IS1 = np.array([IinPo,QinPo,UinPo,VinPo])
ulalume3@0 479 IS2 = np.array([IinPa,QinPa,UinPa,VinPa])
ulalume3@0 480 GT = np.dot(ATP,IS1)
ulalume3@0 481 GR = np.dot(ARP,IS1)
ulalume3@0 482 HT = np.dot(ATP,IS2)
ulalume3@0 483 HR = np.dot(ARP,IS2)
ulalume3@0 484 else:
ulalume3@0 485 IS1e = np.array([IinPo+DiC*QinPoe,DiC*IinPo+QinPoe,ZiC*(CosC*UinPoe+SinC*VinPo),-ZiC*(SinC*UinPoe-CosC*VinPo)])
ulalume3@0 486 IS2e = np.array([IinPa+DiC*QinPae,DiC*IinPa+QinPae,ZiC*(CosC*UinPae+SinC*VinPa),-ZiC*(SinC*UinPae-CosC*VinPa)])
ulalume3@0 487 GT = np.dot(ATPe,IS1e)
ulalume3@0 488 GR = np.dot(ARPe,IS1e)
ulalume3@0 489 HT = np.dot(ATPe,IS2e)
ulalume3@0 490 HR = np.dot(ARPe,IS2e)
ulalume3@0 491 elif (TypeC == 6): # diattenuator calibration +-22.5° rotated_diattenuator_X22x5deg.odt
ulalume3@0 492 # parameters for calibration with aCal
ulalume3@0 493 AT = ATP1*IinP + sqr05*DiC*(ATP1*QinPe + ATP2e*IinP) + (1-0.5*WiC)*(ATP2e*QinPe + ATP3e*UinPe) + ZiC*(sqr05*SinC*(ATP3e*VinP-ATP4*UinPe) + ATP4*CosC*VinP)
ulalume3@0 494 BT = sqr05*DiC*(ATP1*UinPe + ATP3e*IinP) + 0.5*WiC*(ATP2e*UinPe + ATP3e*QinPe) - sqr05*ZiC*SinC*(ATP2e*VinP - ATP4*QinPe)
ulalume3@0 495 AR = ARP1*IinP + sqr05*DiC*(ARP1*QinPe + ARP2e*IinP) + (1-0.5*WiC)*(ARP2e*QinPe + ARP3e*UinPe) + ZiC*(sqr05*SinC*(ARP3e*VinP-ARP4*UinPe) + ARP4*CosC*VinP)
ulalume3@0 496 BR = sqr05*DiC*(ARP1*UinPe + ARP3e*IinP) + 0.5*WiC*(ARP2e*UinPe + ARP3e*QinPe) - sqr05*ZiC*SinC*(ARP2e*VinP - ARP4*QinPe)
ulalume3@0 497 # Correction paremeters for normal measurements; they are independent of LDR
ulalume3@0 498 if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out
ulalume3@0 499 IS1 = np.array([IinPo,QinPo,UinPo,VinPo])
ulalume3@0 500 IS2 = np.array([IinPa,QinPa,UinPa,VinPa])
ulalume3@0 501 GT = np.dot(ATP,IS1)
ulalume3@0 502 GR = np.dot(ARP,IS1)
ulalume3@0 503 HT = np.dot(ATP,IS2)
ulalume3@0 504 HR = np.dot(ARP,IS2)
ulalume3@0 505 else:
ulalume3@0 506 IS1e = np.array([IinPo+DiC*QinPoe,DiC*IinPo+QinPoe,ZiC*(CosC*UinPoe+SinC*VinPo),-ZiC*(SinC*UinPoe-CosC*VinPo)])
ulalume3@0 507 IS2e = np.array([IinPa+DiC*QinPae,DiC*IinPa+QinPae,ZiC*(CosC*UinPae+SinC*VinPa),-ZiC*(SinC*UinPae-CosC*VinPa)])
ulalume3@0 508 GT = np.dot(ATPe,IS1e)
ulalume3@0 509 GR = np.dot(ARPe,IS1e)
ulalume3@0 510 HT = np.dot(ATPe,IS2e)
ulalume3@0 511 HR = np.dot(ARPe,IS2e)
ulalume3@0 512 else:
ulalume3@0 513 print("Calibrator not implemented yet")
ulalume3@0 514 sys.exit()
ulalume3@0 515
ulalume3@0 516 elif LocC == 3: # C before receiver optics Eq.57
ulalume3@0 517
ulalume3@0 518 #S2ge = np.sin(np.deg2rad(2*RotO - 2*RotC))
ulalume3@0 519 #C2ge = np.cos(np.deg2rad(2*RotO - 2*RotC))
ulalume3@0 520 S2e = np.sin(np.deg2rad(2*RotC))
ulalume3@0 521 C2e = np.cos(np.deg2rad(2*RotC))
ulalume3@0 522
ulalume3@0 523 # As with C before the receiver optics (rotated_diattenuator_X22x5deg.odt)
ulalume3@0 524 AF1 = np.array([1,C2g*DiO,S2g*DiO,0])
ulalume3@0 525 AF2 = np.array([C2g*DiO,1-S2g**2*WiO,S2g*C2g*WiO,-S2g*ZiO*SinO])
ulalume3@0 526 AF3 = np.array([S2g*DiO,S2g*C2g*WiO,1-C2g**2*WiO,C2g*ZiO*SinO])
ulalume3@0 527 AF4 = np.array([0,S2g*SinO,-C2g*SinO,CosO])
ulalume3@0 528
ulalume3@0 529 ATF = (ATP1*AF1+ATP2*AF2+ATP3*AF3+ATP4*AF4)
ulalume3@0 530 ARF = (ARP1*AF1+ARP2*AF2+ARP3*AF3+ARP4*AF4)
ulalume3@0 531 ATF2 = ATF[1]
ulalume3@0 532 ATF3 = ATF[2]
ulalume3@0 533 ARF2 = ARF[1]
ulalume3@0 534 ARF3 = ARF[2]
ulalume3@0 535
ulalume3@0 536 # rotated AinF by epsilon
ulalume3@0 537 ATF1 = ATF[0]
ulalume3@0 538 ATF4 = ATF[3]
ulalume3@0 539 ATF2e = C2e*ATF[1] + S2e*ATF[2]
ulalume3@0 540 ATF3e = C2e*ATF[2] - S2e*ATF[1]
ulalume3@0 541 ARF1 = ARF[0]
ulalume3@0 542 ARF4 = ARF[3]
ulalume3@0 543 ARF2e = C2e*ARF[1] + S2e*ARF[2]
ulalume3@0 544 ARF3e = C2e*ARF[2] - S2e*ARF[1]
ulalume3@0 545
ulalume3@0 546 ATFe = np.array([ATF1,ATF2e,ATF3e,ATF4])
ulalume3@0 547 ARFe = np.array([ARF1,ARF2e,ARF3e,ARF4])
ulalume3@0 548
ulalume3@0 549 QinEe = C2e*QinE + S2e*UinE
ulalume3@0 550 UinEe = C2e*UinE - S2e*QinE
ulalume3@0 551
ulalume3@0 552 # Stokes Input Vector before receiver optics Eq. E.19 (after atmosphere F)
ulalume3@0 553 IinF = IinE
ulalume3@0 554 QinF = aCal*QinE
ulalume3@0 555 UinF = -aCal*UinE
ulalume3@0 556 VinF = (1.-2.*aCal)*VinE
ulalume3@0 557
ulalume3@0 558 IinFo = IinE
ulalume3@0 559 QinFo = 0.
ulalume3@0 560 UinFo = 0.
ulalume3@0 561 VinFo = VinE
ulalume3@0 562
ulalume3@0 563 IinFa = 0.
ulalume3@0 564 QinFa = QinE
ulalume3@0 565 UinFa = -UinE
ulalume3@0 566 VinFa = -2.*VinE
ulalume3@0 567
ulalume3@0 568 # Stokes Input Vector before receiver optics rotated by epsilon Eq. C.3
ulalume3@0 569 QinFe = C2e*QinF + S2e*UinF
ulalume3@0 570 UinFe = C2e*UinF - S2e*QinF
ulalume3@0 571 QinFoe = C2e*QinFo + S2e*UinFo
ulalume3@0 572 UinFoe = C2e*UinFo - S2e*QinFo
ulalume3@0 573 QinFae = C2e*QinFa + S2e*UinFa
ulalume3@0 574 UinFae = C2e*UinFa - S2e*QinFa
ulalume3@0 575
ulalume3@0 576 # Calibration signals and Calibration correction K from measurements with LDRCal / aCal
ulalume3@0 577 if (TypeC == 2) or (TypeC == 1): # rotator calibration Eq. C.4
ulalume3@0 578 # parameters for calibration with aCal
ulalume3@0 579 AT = ATF1*IinF + ATF4*h*VinF
ulalume3@0 580 BT = ATF3e*QinF - ATF2e*h*UinF
ulalume3@0 581 AR = ARF1*IinF + ARF4*h*VinF
ulalume3@0 582 BR = ARF3e*QinF - ARF2e*h*UinF
ulalume3@0 583 # Correction paremeters for normal measurements; they are independent of LDR
ulalume3@0 584 if (not RotationErrorEpsilonForNormalMeasurements):
ulalume3@0 585 GT = ATF1*IinE + ATF4*VinE
ulalume3@0 586 GR = ARF1*IinE + ARF4*VinE
ulalume3@0 587 HT = ATF2*QinE - ATF3*UinE - ATF4*2*VinE
ulalume3@0 588 HR = ARF2*QinE - ARF3*UinE - ARF4*2*VinE
ulalume3@0 589 else:
ulalume3@0 590 GT = ATF1*IinE + ATF4*h*VinE
ulalume3@0 591 GR = ARF1*IinE + ARF4*h*VinE
ulalume3@0 592 HT = ATF2e*QinE - ATF3e*h*UinE - ATF4*h*2*VinE
ulalume3@0 593 HR = ARF2e*QinE - ARF3e*h*UinE - ARF4*h*2*VinE
ulalume3@0 594 elif (TypeC == 3) or (TypeC == 4): # linear polariser calibration Eq. C.5
ulalume3@0 595 # p = +45°, m = -45°
ulalume3@0 596 IF1e = np.array([IinF, ZiC*CosC*QinFe, UinFe, ZiC*CosC*VinF])
ulalume3@0 597 IF2e = np.array([DiC*UinFe, -ZiC*SinC*VinF, DiC*IinF, ZiC*SinC*QinFe])
ulalume3@0 598 AT = np.dot(ATFe,IF1e)
ulalume3@0 599 AR = np.dot(ARFe,IF1e)
ulalume3@0 600 BT = np.dot(ATFe,IF2e)
ulalume3@0 601 BR = np.dot(ARFe,IF2e)
ulalume3@0 602
ulalume3@0 603 # Correction paremeters for normal measurements; they are independent of LDR --- the same as for TypeC = 6
ulalume3@0 604 if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out
ulalume3@0 605 IS1 = np.array([IinE,0,0,VinE])
ulalume3@0 606 IS2 = np.array([0,QinE,-UinE,-2*VinE])
ulalume3@0 607 GT = np.dot(ATF,IS1)
ulalume3@0 608 GR = np.dot(ARF,IS1)
ulalume3@0 609 HT = np.dot(ATF,IS2)
ulalume3@0 610 HR = np.dot(ARF,IS2)
ulalume3@0 611 else:
ulalume3@0 612 IS1e = np.array([IinFo+DiC*QinFoe,DiC*IinFo+QinFoe,ZiC*(CosC*UinFoe+SinC*VinFo),-ZiC*(SinC*UinFoe-CosC*VinFo)])
ulalume3@0 613 IS2e = np.array([IinFa+DiC*QinFae,DiC*IinFa+QinFae,ZiC*(CosC*UinFae+SinC*VinFa),-ZiC*(SinC*UinFae-CosC*VinFa)])
ulalume3@0 614 GT = np.dot(ATFe,IS1e)
ulalume3@0 615 GR = np.dot(ARFe,IS1e)
ulalume3@0 616 HT = np.dot(ATFe,IS2e)
ulalume3@0 617 HR = np.dot(ARFe,IS2e)
ulalume3@0 618
ulalume3@0 619 elif (TypeC == 6): # diattenuator calibration +-22.5° rotated_diattenuator_X22x5deg.odt
ulalume3@0 620 # parameters for calibration with aCal
ulalume3@0 621 IF1e = np.array([IinF+sqr05*DiC*QinFe, sqr05*DiC*IinF+(1-0.5*WiC)*QinFe, (1-0.5*WiC)*UinFe+sqr05*ZiC*SinC*VinF, -sqr05*ZiC*SinC*UinFe+ZiC*CosC*VinF])
ulalume3@0 622 IF2e = np.array([sqr05*DiC*UinFe, 0.5*WiC*UinFe-sqr05*ZiC*SinC*VinF, sqr05*DiC*IinF+0.5*WiC*QinFe, sqr05*ZiC*SinC*QinFe])
ulalume3@0 623 AT = np.dot(ATFe,IF1e)
ulalume3@0 624 AR = np.dot(ARFe,IF1e)
ulalume3@0 625 BT = np.dot(ATFe,IF2e)
ulalume3@0 626 BR = np.dot(ARFe,IF2e)
ulalume3@0 627
ulalume3@0 628 # Correction paremeters for normal measurements; they are independent of LDR
ulalume3@0 629 if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out
ulalume3@0 630 #IS1 = np.array([IinE,0,0,VinE])
ulalume3@0 631 #IS2 = np.array([0,QinE,-UinE,-2*VinE])
ulalume3@0 632 IS1 = np.array([IinFo,0,0,VinFo])
ulalume3@0 633 IS2 = np.array([0,QinFa,UinFa,VinFa])
ulalume3@0 634 GT = np.dot(ATF,IS1)
ulalume3@0 635 GR = np.dot(ARF,IS1)
ulalume3@0 636 HT = np.dot(ATF,IS2)
ulalume3@0 637 HR = np.dot(ARF,IS2)
ulalume3@0 638 else:
ulalume3@0 639 IS1e = np.array([IinFo+DiC*QinFoe,DiC*IinFo+QinFoe,ZiC*(CosC*UinFoe+SinC*VinFo),-ZiC*(SinC*UinFoe-CosC*VinFo)])
ulalume3@0 640 IS2e = np.array([IinFa+DiC*QinFae,DiC*IinFa+QinFae,ZiC*(CosC*UinFae+SinC*VinFa),-ZiC*(SinC*UinFae-CosC*VinFa)])
ulalume3@0 641 #IS1e = np.array([IinFo,0,0,VinFo])
ulalume3@0 642 #IS2e = np.array([0,QinFae,UinFae,VinFa])
ulalume3@0 643 GT = np.dot(ATFe,IS1e)
ulalume3@0 644 GR = np.dot(ARFe,IS1e)
ulalume3@0 645 HT = np.dot(ATFe,IS2e)
ulalume3@0 646 HR = np.dot(ARFe,IS2e)
ulalume3@0 647
ulalume3@0 648 else:
ulalume3@0 649 print('Calibrator not implemented yet')
ulalume3@0 650 sys.exit()
ulalume3@0 651
ulalume3@0 652 elif LocC == 2: # C behind emitter optics Eq.57 -------------------------------------------------------
ulalume3@0 653 #print("Calibrator location not implemented yet")
ulalume3@0 654 S2e = np.sin(np.deg2rad(2*RotC))
ulalume3@0 655 C2e = np.cos(np.deg2rad(2*RotC))
ulalume3@0 656
ulalume3@0 657 # AS with C before the receiver optics (see document rotated_diattenuator_X22x5deg.odt)
ulalume3@0 658 AF1 = np.array([1,C2g*DiO,S2g*DiO,0])
ulalume3@0 659 AF2 = np.array([C2g*DiO,1-S2g**2*WiO,S2g*C2g*WiO,-S2g*ZiO*SinO])
ulalume3@0 660 AF3 = np.array([S2g*DiO, S2g*C2g*WiO, 1-C2g**2*WiO, C2g*ZiO*SinO])
ulalume3@0 661 AF4 = np.array([0, S2g*SinO, -C2g*SinO, CosO])
ulalume3@0 662
ulalume3@0 663 ATF = (ATP1*AF1+ATP2*AF2+ATP3*AF3+ATP4*AF4)
ulalume3@0 664 ARF = (ARP1*AF1+ARP2*AF2+ARP3*AF3+ARP4*AF4)
ulalume3@0 665 ATF1 = ATF[0]
ulalume3@0 666 ATF2 = ATF[1]
ulalume3@0 667 ATF3 = ATF[2]
ulalume3@0 668 ATF4 = ATF[3]
ulalume3@0 669 ARF1 = ARF[0]
ulalume3@0 670 ARF2 = ARF[1]
ulalume3@0 671 ARF3 = ARF[2]
ulalume3@0 672 ARF4 = ARF[3]
ulalume3@0 673
ulalume3@0 674 # AS with C behind the emitter
ulalume3@0 675 # terms without aCal
ulalume3@0 676 ATE1o, ARE1o = ATF1, ARF1
ulalume3@0 677 ATE2o, ARE2o = 0., 0.
ulalume3@0 678 ATE3o, ARE3o = 0., 0.
ulalume3@0 679 ATE4o, ARE4o = ATF4, ARF4
ulalume3@0 680 # terms with aCal
ulalume3@0 681 ATE1a, ARE1a = 0. , 0.
ulalume3@0 682 ATE2a, ARE2a = ATF2, ARF2
ulalume3@0 683 ATE3a, ARE3a = -ATF3, -ARF3
ulalume3@0 684 ATE4a, ARE4a = -2*ATF4, -2*ARF4
ulalume3@0 685 # rotated AinEa by epsilon
ulalume3@0 686 ATE2ae = C2e*ATF2 + S2e*ATF3
ulalume3@0 687 ATE3ae = -S2e*ATF2 - C2e*ATF3
ulalume3@0 688 ARE2ae = C2e*ARF2 + S2e*ARF3
ulalume3@0 689 ARE3ae = -S2e*ARF2 - C2e*ARF3
ulalume3@0 690
ulalume3@0 691 ATE1 = ATE1o
ulalume3@0 692 ATE2e = aCal*ATE2ae
ulalume3@0 693 ATE3e = aCal*ATE3ae
ulalume3@0 694 ATE4 = (1-2*aCal)*ATF4
ulalume3@0 695 ARE1 = ARE1o
ulalume3@0 696 ARE2e = aCal*ARE2ae
ulalume3@0 697 ARE3e = aCal*ARE3ae
ulalume3@0 698 ARE4 = (1-2*aCal)*ARF4
ulalume3@0 699
ulalume3@0 700 # rotated IinE
ulalume3@0 701 QinEe = C2e*QinE + S2e*UinE
ulalume3@0 702 UinEe = C2e*UinE - S2e*QinE
ulalume3@0 703
ulalume3@0 704 # Calibration signals and Calibration correction K from measurements with LDRCal / aCal
ulalume3@0 705 if (TypeC == 2) or (TypeC == 1): # +++++++++ rotator calibration Eq. C.4
ulalume3@0 706 AT = ATE1o*IinE + (ATE4o+aCal*ATE4a)*h*VinE
ulalume3@0 707 BT = aCal * (ATE3ae*QinEe - ATE2ae*h*UinEe)
ulalume3@0 708 AR = ARE1o*IinE + (ARE4o+aCal*ARE4a)*h*VinE
ulalume3@0 709 BR = aCal * (ARE3ae*QinEe - ARE2ae*h*UinEe)
ulalume3@0 710
ulalume3@0 711 # Correction paremeters for normal measurements; they are independent of LDR
ulalume3@0 712 if (not RotationErrorEpsilonForNormalMeasurements):
ulalume3@0 713 # Stokes Input Vector before receiver optics Eq. E.19 (after atmosphere F)
ulalume3@0 714 GT = ATE1o*IinE + ATE4o*h*VinE
ulalume3@0 715 GR = ARE1o*IinE + ARE4o*h*VinE
ulalume3@0 716 HT = ATE2a*QinE + ATE3a*h*UinEe + ATE4a*h*VinE
ulalume3@0 717 HR = ARE2a*QinE + ARE3a*h*UinEe + ARE4a*h*VinE
ulalume3@0 718 else:
ulalume3@0 719 GT = ATE1o*IinE + ATE4o*h*VinE
ulalume3@0 720 GR = ARE1o*IinE + ARE4o*h*VinE
ulalume3@0 721 HT = ATE2ae*QinE + ATE3ae*h*UinEe + ATE4a*h*VinE
ulalume3@0 722 HR = ARE2ae*QinE + ARE3ae*h*UinEe + ARE4a*h*VinE
ulalume3@0 723
ulalume3@0 724 elif (TypeC == 3) or (TypeC == 4): # +++++++++ linear polariser calibration Eq. C.5
ulalume3@0 725 # p = +45°, m = -45°
ulalume3@0 726 AT = ATE1*IinE + ZiC*CosC*(ATE2e*QinEe + ATE4*VinE) + ATE3e*UinEe
ulalume3@0 727 BT = DiC*(ATE1*UinEe + ATE3e*IinE) + ZiC*SinC*(ATE4*QinEe - ATE2e*VinE)
ulalume3@0 728 AR = ARE1*IinE + ZiC*CosC*(ARE2e*QinEe + ARE4*VinE) + ARE3e*UinEe
ulalume3@0 729 BR = DiC*(ARE1*UinEe + ARE3e*IinE) + ZiC*SinC*(ARE4*QinEe - ARE2e*VinE)
ulalume3@0 730
ulalume3@0 731 # Correction paremeters for normal measurements; they are independent of LDR
ulalume3@0 732 if (not RotationErrorEpsilonForNormalMeasurements):
ulalume3@0 733 # Stokes Input Vector before receiver optics Eq. E.19 (after atmosphere F)
ulalume3@0 734 GT = ATE1o*IinE + ATE4o*VinE
ulalume3@0 735 GR = ARE1o*IinE + ARE4o*VinE
ulalume3@0 736 HT = ATE2a*QinE + ATE3a*UinE + ATE4a*VinE
ulalume3@0 737 HR = ARE2a*QinE + ARE3a*UinE + ARE4a*VinE
ulalume3@0 738 else:
ulalume3@0 739 D = IinE + DiC*QinEe
ulalume3@0 740 A = DiC*IinE + QinEe
ulalume3@0 741 B = ZiC*(CosC*UinEe + SinC*VinE)
ulalume3@0 742 C = -ZiC*(SinC*UinEe - CosC*VinE)
ulalume3@0 743 GT = ATE1o*D + ATE4o*C
ulalume3@0 744 GR = ARE1o*D + ARE4o*C
ulalume3@0 745 HT = ATE2a*A + ATE3a*B + ATE4a*C
ulalume3@0 746 HR = ARE2a*A + ARE3a*B + ARE4a*C
ulalume3@0 747
ulalume3@0 748 elif (TypeC == 6): # real HWP calibration +-22.5° rotated_diattenuator_X22x5deg.odt
ulalume3@0 749 # p = +22.5°, m = -22.5°
ulalume3@0 750 IE1e = np.array([IinE+sqr05*DiC*QinEe, sqr05*DiC*IinE+(1-0.5*WiC)*QinEe, (1-0.5*WiC)*UinEe+sqr05*ZiC*SinC*VinE, -sqr05*ZiC*SinC*UinEe+ZiC*CosC*VinE])
ulalume3@0 751 IE2e = np.array([sqr05*DiC*UinEe, 0.5*WiC*UinEe-sqr05*ZiC*SinC*VinE, sqr05*DiC*IinE+0.5*WiC*QinEe, sqr05*ZiC*SinC*QinEe])
ulalume3@0 752 ATEe = np.array([ATE1,ATE2e,ATE3e,ATE4])
ulalume3@0 753 AREe = np.array([ARE1,ARE2e,ARE3e,ARE4])
ulalume3@0 754 AT = np.dot(ATEe,IE1e)
ulalume3@0 755 AR = np.dot(AREe,IE1e)
ulalume3@0 756 BT = np.dot(ATEe,IE2e)
ulalume3@0 757 BR = np.dot(AREe,IE2e)
ulalume3@0 758
ulalume3@0 759 # Correction paremeters for normal measurements; they are independent of LDR
ulalume3@0 760 if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out
ulalume3@0 761 GT = ATE1o*IinE + ATE4o*VinE
ulalume3@0 762 GR = ARE1o*IinE + ARE4o*VinE
ulalume3@0 763 HT = ATE2a*QinE + ATE3a*UinE + ATE4a*VinE
ulalume3@0 764 HR = ARE2a*QinE + ARE3a*UinE + ARE4a*VinE
ulalume3@0 765 else:
ulalume3@0 766 D = IinE + DiC*QinEe
ulalume3@0 767 A = DiC*IinE + QinEe
ulalume3@0 768 B = ZiC*(CosC*UinEe + SinC*VinE)
ulalume3@0 769 C = -ZiC*(SinC*UinEe - CosC*VinE)
ulalume3@0 770 GT = ATE1o*D + ATE4o*C
ulalume3@0 771 GR = ARE1o*D + ARE4o*C
ulalume3@0 772 HT = ATE2a*A + ATE3a*B + ATE4a*C
ulalume3@0 773 HR = ARE2a*A + ARE3a*B + ARE4a*C
ulalume3@0 774
ulalume3@0 775 else:
ulalume3@0 776 print('Calibrator not implemented yet')
ulalume3@0 777 sys.exit()
ulalume3@0 778
ulalume3@0 779 else:
ulalume3@0 780 print("Calibrator location not implemented yet")
ulalume3@0 781 sys.exit()
ulalume3@0 782
ulalume3@0 783 # Determination of the correction K of the calibration factor
ulalume3@0 784 IoutTp = TaT*TiT*TiO*TiE*(AT + BT)
ulalume3@0 785 IoutTm = TaT*TiT*TiO*TiE*(AT - BT)
ulalume3@0 786 IoutRp = TaR*TiR*TiO*TiE*(AR + BR)
ulalume3@0 787 IoutRm = TaR*TiR*TiO*TiE*(AR - BR)
ulalume3@0 788
ulalume3@0 789 # --- Results and Corrections; electronic etaR and etaT are assumed to be 1
ulalume3@0 790 Etapx = IoutRp/IoutTp
ulalume3@0 791 Etamx = IoutRm/IoutTm
ulalume3@0 792 Etax = (Etapx*Etamx)**0.5
ulalume3@0 793
ulalume3@0 794 Eta = (TaR*TiR)/(TaT*TiT) # Eta = Eta*/K Eq. 84
ulalume3@0 795 K = Etax / Eta
ulalume3@0 796
ulalume3@0 797 # For comparison with Volkers Libreoffice Müller Matrix spreadsheet
ulalume3@0 798 #Eta_test_p = (IoutRp/IoutTp)
ulalume3@0 799 #Eta_test_m = (IoutRm/IoutTm)
ulalume3@0 800 #Eta_test = (Eta_test_p*Eta_test_m)**0.5
ulalume3@0 801
ulalume3@0 802 # ----- Forward simulated signals and LDRsim with atrue; from input file
ulalume3@0 803 It = TaT*TiT*TiO*TiE*(GT+atrue*HT)
ulalume3@0 804 Ir = TaR*TiR*TiO*TiE*(GR+atrue*HR)
ulalume3@0 805 # LDRsim = 1/Eta*Ir/It # simulated LDR* with Y from input file
ulalume3@0 806 LDRsim = Ir/It # simulated uncorrected LDR with Y from input file
ulalume3@0 807 # Corrected LDRsimCorr from forward simulated LDRsim (atrue)
ulalume3@0 808 # LDRsimCorr = (1./Eta*LDRsim*(GT+HT)-(GR+HR))/((GR-HR)-1./Eta*LDRsim*(GT-HT))
ulalume3@0 809 if Y == -1.:
ulalume3@0 810 LDRsimx = 1./LDRsim
ulalume3@0 811 else:
ulalume3@0 812 LDRsimx = LDRsim
ulalume3@0 813
ulalume3@0 814 # The following is correct without doubt
ulalume3@0 815 #LDRCorr = (LDRsim*K/Etax*(GT+HT)-(GR+HR))/((GR-HR)-LDRsim*K/Etax*(GT-HT))
ulalume3@0 816
ulalume3@0 817 # The following is a test whether the equations for calibration Etax and normal signal (GHK, LDRsim) are consistent
ulalume3@0 818 LDRCorr = (LDRsim/Eta*(GT+HT)-(GR+HR))/((GR-HR)-LDRsim*K/Etax*(GT-HT))
ulalume3@0 819
ulalume3@0 820 TTa = TiT*TaT #*ATP1
ulalume3@0 821 TRa = TiR*TaR #*ARP1
ulalume3@0 822
ulalume3@0 823 F11sim = 1/(TiO*TiE)*((HR*Etax/K*It/TTa-HT*Ir/TRa)/(HR*GT-HT*GR)) # IL = 1, Etat = Etar = 1
ulalume3@0 824
ulalume3@0 825 return (GT, HT, GR, HR, K, Eta, LDRsimx, LDRCorr, DTa, DRa, TTa, TRa, F11sim)
ulalume3@0 826 # *******************************************************************************************************************************
ulalume3@0 827
ulalume3@0 828 # --- CALC truth
ulalume3@0 829 GT0, HT0, GR0, HR0, K0, Eta0, LDRsimx, LDRCorr, DTa0, DRa0, TTa0, TRa0, F11sim0 = Calc(RotL0, RotE0, RetE0, DiE0, RotO0, RetO0, DiO0, RotC0, RetC0, DiC0, TP0, TS0, RP0, RS0, ERaT0, RotaT0, RetT0, ERaR0, RotaR0, RetR0, LDRCal0)
ulalume3@0 830
volker@13 831 # --- Print parameters to console and output file
volker@13 832 with open('output_files\output_' + LID + '.dat', 'w') as f:
ulalume3@0 833 with redirect_stdout(f):
ulalume3@0 834 print("From ", dname)
ulalume3@0 835 print("Running ", fname)
ulalume3@0 836 print("Reading input file ", InputFile) #, " for Lidar system :", EID, ", ", LID)
ulalume3@0 837 print("for Lidar system: ", EID, ", ", LID)
ulalume3@0 838 # --- Print iput information*********************************
ulalume3@0 839 print(" --- Input parameters: value ±error / ±steps ----------------------")
ulalume3@0 840 print("{0:8} {1:8} {2:8.5f}; {3:8} {4:7.4f}±{5:7.4f}/{6:2d}".format("Laser: ", "DOLP = ", bL, " rotation alpha = ", RotL0, dRotL, nRotL))
ulalume3@0 841 print(" Diatt., Tunpol, Retard., Rotation (deg)")
ulalume3@0 842 print("{0:12} {1:7.4f}±{2:7.4f}/{8:2d}, {3:7.4f}, {4:3.0f}±{5:3.0f}/{9:2d}, {6:7.4f}±{7:7.4f}/{10:2d}".format("Emitter ", DiE0, dDiE, TiE, RetE0, dRetE, RotE0, dRotE, nDiE, nRetE, nRotE))
ulalume3@0 843 print("{0:12} {1:7.4f}±{2:7.4f}/{8:2d}, {3:7.4f}, {4:3.0f}±{5:3.0f}/{9:2d}, {6:7.4f}±{7:7.4f}/{10:2d}".format("Receiver ", DiO0, dDiO, TiO, RetO0, dRetO, RotO0, dRotO, nDiO, nRetO, nRotO))
ulalume3@0 844 print("{0:12} {1:7.4f}±{2:7.4f}/{8:2d}, {3:7.4f}, {4:3.0f}±{5:3.0f}/{9:2d}, {6:7.4f}±{7:7.4f}/{10:2d}".format("Calibrator ", DiC0, dDiC, TiC, RetC0, dRetC, RotC0, dRotC, nDiC, nRetC, nRotC))
ulalume3@0 845 print("{0:12}".format(" --- Pol.-filter ---"))
ulalume3@0 846 print("{0:12}{1:7.4f}±{2:7.4f}/{3:2d}, {4:7.4f}±{5:7.4f}/{6:2d}".format("ERT, ERR :", ERaT0, dERaT, nERaT, ERaR0, dERaR, nERaR))
ulalume3@0 847 print("{0:12}{1:7.4f}±{2:7.4f}/{3:2d}, {4:7.4f}±{5:7.4f}/{6:2d}".format("RotaT , RotaR :", RotaT0, dRotaT, nRotaT, RotaR0,dRotaR,nRotaR))
ulalume3@0 848 print("{0:12}".format(" --- PBS ---"))
ulalume3@0 849 print("{0:12}{1:7.4f}±{2:7.4f}/{9:2d}, {3:7.4f}±{4:7.4f}/{10:2d}, {5:7.4f}±{6:7.4f}/{11:2d},{7:7.4f}±{8:7.4f}/{12:2d}".format("TP,TS,RP,RS :", TP0, dTP, TS0, dTS, RP0, dRP, RS0, dRS, nTP, nTS, nRP, nRS))
ulalume3@0 850 print("{0:12}{1:7.4f},{2:7.4f}, {3:7.4f},{4:7.4f}, {5:1.0f}".format("DT,TT,DR,TR,Y :", DiT, TiT, DiR, TiR, Y))
ulalume3@0 851 print("{0:12}".format(" --- Combined PBS + Pol.-filter ---"))
volker@13 852 print("{0:12}{1:7.4f},{2:7.4f}, {3:7.4f},{4:7.4f}".format("DT,TT,DR,TR :", DTa0, TTa0, DRa0, TRa0))
ulalume3@0 853 print()
ulalume3@0 854 print("Rotation Error Epsilon For Normal Measurements = ", RotationErrorEpsilonForNormalMeasurements)
volker@13 855 print(Type[TypeC], Loc[LocC])
volker@13 856 print("Parallel signal detected in", dY[int(Y+1)])
volker@13 857 print("RS_RP_depend_on_TS_TP = ", RS_RP_depend_on_TS_TP)
ulalume3@0 858 # end of print actual system parameters
ulalume3@0 859 # ******************************************************************************
ulalume3@0 860
ulalume3@0 861 #print()
ulalume3@0 862 #print(" --- LDRCal during calibration | simulated and corrected LDRs -------------")
ulalume3@0 863 #print("{0:8} |{1:8}->{2:8},{3:9}->{4:9} |{5:8}->{6:8}".format(" LDRCal"," LDRtrue", " LDRsim"," LDRtrue2", " LDRsim2", " LDRmeas", " LDRcorr"))
ulalume3@0 864 #print("{0:8.5f} |{1:8.5f}->{2:8.5f},{3:9.5f}->{4:9.5f} |{5:8.5f}->{6:8.5f}".format(LDRCal, LDRtrue, LDRsim, LDRtrue2, LDRsim2, LDRmeas, LDRCorr))
ulalume3@0 865 #print("{0:8} |{1:8}->{2:8}->{3:8}".format(" LDRCal"," LDRtrue", " LDRsimx", " LDRcorr"))
ulalume3@0 866 #print("{0:6.3f}±{1:5.3f}/{2:2d}|{3:8.5f}->{4:8.5f}->{5:8.5f}".format(LDRCal0, dLDRCal, nLDRCal, LDRtrue, LDRsimx, LDRCorr))
ulalume3@0 867 #print("{0:8} |{1:8}->{2:8}->{3:8}".format(" LDRCal"," LDRtrue", " LDRsimx", " LDRcorr"))
ulalume3@0 868 #print(" --- LDRCal during calibration")
ulalume3@0 869 print("{0:26}: {1:6.3f}±{2:5.3f}/{3:2d}".format("LDRCal during calibration", LDRCal0, dLDRCal, nLDRCal))
ulalume3@0 870
ulalume3@0 871 #print("{0:8}={1:8.5f};{2:8}={3:8.5f}".format(" IinP",IinP," F11sim",F11sim))
ulalume3@0 872 print()
ulalume3@0 873
ulalume3@0 874 K0List = np.zeros(3)
ulalume3@0 875 LDRsimxList = np.zeros(3)
ulalume3@0 876 LDRCalList = 0.004, 0.2, 0.45
ulalume3@0 877 for i,LDRCal in enumerate(LDRCalList):
ulalume3@0 878 GT0, HT0, GR0, HR0, K0, Eta0, LDRsimx, LDRCorr, DTa0, DRa0, TTa0, TRa0, F11sim0 = Calc(RotL0, RotE0, RetE0, DiE0, RotO0, RetO0, DiO0, RotC0, RetC0, DiC0, TP0, TS0, RP0, RS0, ERaT0, RotaT0, RetT0, ERaR0, RotaR0, RetR0, LDRCal)
ulalume3@0 879 K0List[i] = K0
ulalume3@0 880 LDRsimxList[i] = LDRsimx
ulalume3@0 881
volker@13 882 print('========================================================================')
volker@13 883 print("{0:8},{1:8},{2:8},{3:8},{4:9},{5:8},{6:9}".format(" GR", " GT", " HR", " HT", " K(0.004)", " K(0.2)", " K(0.45)"))
ulalume3@0 884 print("{0:8.5f},{1:8.5f},{2:8.5f},{3:8.5f},{4:9.5f},{5:9.5f},{6:9.5f}".format(GR0, GT0, HR0, HT0, K0List[0], K0List[1], K0List[2]))
ulalume3@0 885 print('========================================================================')
ulalume3@0 886
ulalume3@0 887 print("{0:9},{1:9},{2:9}".format(" LDRtrue", " LDRsimx", " LDRCorr"))
ulalume3@0 888 LDRtrueList = 0.004, 0.02, 0.2, 0.45
ulalume3@0 889 for i,LDRtrue in enumerate(LDRtrueList):
ulalume3@0 890 GT0, HT0, GR0, HR0, K0, Eta0, LDRsimx, LDRCorr, DTa0, DRa0, TTa0, TRa0, F11sim0 = Calc(RotL0, RotE0, RetE0, DiE0, RotO0, RetO0, DiO0, RotC0, RetC0, DiC0, TP0, TS0, RP0, RS0, ERaT0, RotaT0, RetT0, ERaR0, RotaR0, RetR0, LDRCal0)
ulalume3@0 891 print("{0:9.5f},{1:9.5f},{2:9.5f}".format(LDRtrue, LDRsimx, LDRCorr))
ulalume3@0 892
ulalume3@0 893
volker@13 894 file = open('output_files\output_' + LID + '.dat', 'r')
ulalume3@0 895 print (file.read())
ulalume3@0 896 file.close()
ulalume3@0 897
ulalume3@0 898 '''
ulalume3@0 899 if(PrintToOutputFile):
ulalume3@0 900 f = open('output_ver7.dat', 'w')
ulalume3@0 901 old_target = sys.stdout
ulalume3@0 902 sys.stdout = f
ulalume3@0 903
ulalume3@0 904 print("something")
ulalume3@0 905
ulalume3@0 906 if(PrintToOutputFile):
ulalume3@0 907 sys.stdout.flush()
ulalume3@0 908 f.close
ulalume3@0 909 sys.stdout = old_target
ulalume3@0 910 '''
ulalume3@0 911 # --- CALC again truth with LDRCal0 to reset all 0-values
ulalume3@0 912 GT0, HT0, GR0, HR0, K0, Eta0, LDRsimx, LDRCorr, DTa0, DRa0, TTa0, TRa0, F11sim0 = Calc(RotL0, RotE0, RetE0, DiE0, RotO0, RetO0, DiO0, RotC0, RetC0, DiC0, TP0, TS0, RP0, RS0, ERaT0, RotaT0, RetT0, ERaR0, RotaR0, RetR0, LDRCal0)
ulalume3@0 913
volker@13 914 # --- Start Errors calculation with variable parameters ------------------------------------------------------------------
ulalume3@0 915
ulalume3@0 916 iN = -1
ulalume3@0 917 N = ((nRotL*2+1)*
ulalume3@0 918 (nRotE*2+1)*(nRetE*2+1)*(nDiE*2+1)*
ulalume3@0 919 (nRotO*2+1)*(nRetO*2+1)*(nDiO*2+1)*
ulalume3@0 920 (nRotC*2+1)*(nRetC*2+1)*(nDiC*2+1)*
ulalume3@0 921 (nTP*2+1)*(nTS*2+1)*(nRP*2+1)*(nRS*2+1)*(nERaT*2+1)*(nERaR*2+1)*
ulalume3@0 922 (nRotaT*2+1)*(nRotaR*2+1)*(nRetT*2+1)*(nRetR*2+1)*(nLDRCal*2+1))
ulalume3@0 923 print("N = ",N ," ", end="")
ulalume3@0 924
ulalume3@0 925 if N > 1e6:
ulalume3@0 926 if user_yes_no_query('Warning: processing ' + str(N) + ' samples will take very long. Do you want to proceed?') == 0: sys.exit()
ulalume3@0 927 if N > 5e6:
ulalume3@0 928 if user_yes_no_query('Warning: the memory required for ' + str(N) + ' samples might be ' + '{0:5.1f}'.format(N/4e6) + ' GB. Do you anyway want to proceed?') == 0: sys.exit()
ulalume3@0 929
ulalume3@0 930 #if user_yes_no_query('Warning: processing' + str(N) + ' samples will take very long. Do you want to proceed?') == 0: sys.exit()
ulalume3@0 931
ulalume3@0 932 # --- Arrays for plotting ------
ulalume3@0 933 LDRmin = np.zeros(5)
ulalume3@0 934 LDRmax = np.zeros(5)
ulalume3@0 935 F11min = np.zeros(5)
ulalume3@0 936 F11max = np.zeros(5)
ulalume3@0 937
ulalume3@0 938 LDRrange = np.zeros(5)
ulalume3@0 939 LDRrange = 0.004, 0.02, 0.1, 0.3, 0.45
ulalume3@0 940 #aLDRsimx = np.zeros(N)
ulalume3@0 941 #aLDRsimx2 = np.zeros(N)
ulalume3@0 942 #aLDRcorr = np.zeros(N)
ulalume3@0 943 #aLDRcorr2 = np.zeros(N)
ulalume3@0 944 aERaT = np.zeros(N)
ulalume3@0 945 aERaR = np.zeros(N)
ulalume3@0 946 aRotaT = np.zeros(N)
ulalume3@0 947 aRotaR = np.zeros(N)
ulalume3@0 948 aRetT = np.zeros(N)
ulalume3@0 949 aRetR = np.zeros(N)
ulalume3@0 950 aTP = np.zeros(N)
ulalume3@0 951 aTS = np.zeros(N)
ulalume3@0 952 aRP = np.zeros(N)
ulalume3@0 953 aRS = np.zeros(N)
ulalume3@0 954 aDiE = np.zeros(N)
ulalume3@0 955 aDiO = np.zeros(N)
ulalume3@0 956 aDiC = np.zeros(N)
ulalume3@0 957 aRotC = np.zeros(N)
ulalume3@0 958 aRetC = np.zeros(N)
ulalume3@0 959 aRotL = np.zeros(N)
ulalume3@0 960 aRetE = np.zeros(N)
ulalume3@0 961 aRotE = np.zeros(N)
ulalume3@0 962 aRetO = np.zeros(N)
ulalume3@0 963 aRotO = np.zeros(N)
ulalume3@0 964 aLDRCal = np.zeros(N)
ulalume3@0 965 aA = np.zeros((5,N))
ulalume3@0 966 aX = np.zeros((5,N))
ulalume3@0 967 aF11corr = np.zeros((5,N))
ulalume3@0 968
ulalume3@0 969 atime = clock()
ulalume3@0 970 dtime = clock()
ulalume3@0 971
ulalume3@0 972 # --- Calc Error signals
ulalume3@0 973 #GT, HT, GR, HR, K, Eta, LDRsim = Calc(RotL, RotE, RetE, DiE, RotO, RetO, DiO, RotC, RetC, DiC, TP, TS)
ulalume3@0 974 # ---- Do the calculations of bra-ket vectors
ulalume3@0 975 h = -1. if TypeC == 2 else 1
ulalume3@0 976
ulalume3@0 977 # from input file: measured LDRm and true LDRtrue, LDRtrue2 =>
ulalume3@0 978 ameas = (1.-LDRmeas)/(1+LDRmeas)
ulalume3@0 979 atrue = (1.-LDRtrue)/(1+LDRtrue)
ulalume3@0 980 atrue2 = (1.-LDRtrue2)/(1+LDRtrue2)
ulalume3@0 981
ulalume3@0 982 for iLDRCal in range(-nLDRCal,nLDRCal+1):
ulalume3@0 983 # from input file: assumed LDRCal for calibration measurements
ulalume3@0 984 LDRCal = LDRCal0
ulalume3@0 985 if nLDRCal > 0: LDRCal = LDRCal0 + iLDRCal*dLDRCal/nLDRCal
ulalume3@0 986
ulalume3@0 987 GT0, HT0, GR0, HR0, K0, Eta0, LDRsimx, LDRCorr, DTa0, DRa0, TTa0, TRa0, F11sim0 = Calc(RotL0, RotE0, RetE0, DiE0, RotO0, RetO0, DiO0, RotC0, RetC0, DiC0, TP0, TS0, RP0, RS0, ERaT0, RotaT0, RetT0, ERaR0, RotaR0, RetR0, LDRCal)
ulalume3@0 988 aCal = (1.-LDRCal)/(1+LDRCal)
ulalume3@0 989 for iRotL, iRotE, iRetE, iDiE \
ulalume3@0 990 in [(iRotL,iRotE,iRetE,iDiE)
ulalume3@0 991 for iRotL in range(-nRotL,nRotL+1)
ulalume3@0 992 for iRotE in range(-nRotE,nRotE+1)
ulalume3@0 993 for iRetE in range(-nRetE,nRetE+1)
ulalume3@0 994 for iDiE in range(-nDiE,nDiE+1)]:
ulalume3@0 995
ulalume3@0 996 if nRotL > 0: RotL = RotL0 + iRotL*dRotL/nRotL
ulalume3@0 997 if nRotE > 0: RotE = RotE0 + iRotE*dRotE/nRotE
ulalume3@0 998 if nRetE > 0: RetE = RetE0 + iRetE*dRetE/nRetE
ulalume3@0 999 if nDiE > 0: DiE = DiE0 + iDiE*dDiE/nDiE
ulalume3@0 1000
ulalume3@0 1001 # angles of emitter and laser and calibrator and receiver optics
ulalume3@0 1002 # RotL = alpha, RotE = beta, RotO = gamma, RotC = epsilon
ulalume3@0 1003 S2a = np.sin(2*np.deg2rad(RotL))
ulalume3@0 1004 C2a = np.cos(2*np.deg2rad(RotL))
ulalume3@0 1005 S2b = np.sin(2*np.deg2rad(RotE))
ulalume3@0 1006 C2b = np.cos(2*np.deg2rad(RotE))
ulalume3@0 1007 S2ab = np.sin(np.deg2rad(2*RotL-2*RotE))
ulalume3@0 1008 C2ab = np.cos(np.deg2rad(2*RotL-2*RotE))
ulalume3@0 1009
ulalume3@0 1010 # Laser with Degree of linear polarization DOLP = bL
ulalume3@0 1011 IinL = 1.
ulalume3@0 1012 QinL = bL
ulalume3@0 1013 UinL = 0.
ulalume3@0 1014 VinL = (1. - bL**2)**0.5
ulalume3@0 1015
ulalume3@0 1016 # Stokes Input Vector rotation Eq. E.4
ulalume3@0 1017 A = C2a*QinL - S2a*UinL
ulalume3@0 1018 B = S2a*QinL + C2a*UinL
ulalume3@0 1019 # Stokes Input Vector rotation Eq. E.9
ulalume3@0 1020 C = C2ab*QinL - S2ab*UinL
ulalume3@0 1021 D = S2ab*QinL + C2ab*UinL
ulalume3@0 1022
ulalume3@0 1023 # emitter optics
ulalume3@0 1024 CosE = np.cos(np.deg2rad(RetE))
ulalume3@0 1025 SinE = np.sin(np.deg2rad(RetE))
ulalume3@0 1026 ZiE = (1. - DiE**2)**0.5
ulalume3@0 1027 WiE = (1. - ZiE*CosE)
ulalume3@0 1028
ulalume3@0 1029 # Stokes Input Vector after emitter optics equivalent to Eq. E.9 with already rotated input vector from Eq. E.4
ulalume3@0 1030 # b = beta
ulalume3@0 1031 IinE = (IinL + DiE*C)
ulalume3@0 1032 QinE = (C2b*DiE*IinL + A + S2b*(WiE*D - ZiE*SinE*VinL))
ulalume3@0 1033 UinE = (S2b*DiE*IinL + B - C2b*(WiE*D - ZiE*SinE*VinL))
ulalume3@0 1034 VinE = (-ZiE*SinE*D + ZiE*CosE*VinL)
ulalume3@0 1035
ulalume3@0 1036 #-------------------------
ulalume3@0 1037 # F11 assuemd to be = 1 => measured: F11m = IinP / IinE with atrue
ulalume3@0 1038 #F11sim = (IinE + DiO*atrue*(C2g*QinE - S2g*UinE))/IinE
ulalume3@0 1039 #-------------------------
ulalume3@0 1040
ulalume3@0 1041 for iRotO, iRetO, iDiO, iRotC, iRetC, iDiC, iTP, iTS, iRP, iRS, iERaT, iRotaT, iRetT, iERaR, iRotaR, iRetR \
ulalume3@0 1042 in [(iRotO,iRetO,iDiO,iRotC,iRetC,iDiC,iTP,iTS,iRP,iRS,iERaT,iRotaT,iRetT,iERaR,iRotaR,iRetR )
ulalume3@0 1043 for iRotO in range(-nRotO,nRotO+1)
ulalume3@0 1044 for iRetO in range(-nRetO,nRetO+1)
ulalume3@0 1045 for iDiO in range(-nDiO,nDiO+1)
ulalume3@0 1046 for iRotC in range(-nRotC,nRotC+1)
ulalume3@0 1047 for iRetC in range(-nRetC,nRetC+1)
ulalume3@0 1048 for iDiC in range(-nDiC,nDiC+1)
ulalume3@0 1049 for iTP in range(-nTP,nTP+1)
ulalume3@0 1050 for iTS in range(-nTS,nTS+1)
ulalume3@0 1051 for iRP in range(-nRP,nRP+1)
ulalume3@0 1052 for iRS in range(-nRS,nRS+1)
ulalume3@0 1053 for iERaT in range(-nERaT,nERaT+1)
ulalume3@0 1054 for iRotaT in range(-nRotaT,nRotaT+1)
ulalume3@0 1055 for iRetT in range(-nRetT,nRetT+1)
ulalume3@0 1056 for iERaR in range(-nERaR,nERaR+1)
ulalume3@0 1057 for iRotaR in range(-nRotaR,nRotaR+1)
ulalume3@0 1058 for iRetR in range(-nRetR,nRetR+1)]:
ulalume3@0 1059
ulalume3@0 1060 iN = iN + 1
ulalume3@0 1061 if (iN == 10001):
ulalume3@0 1062 ctime = clock()
ulalume3@0 1063 print(" estimated time ", "{0:4.2f}".format(N/10000 * (ctime-atime)), "sec ") #, end="")
ulalume3@0 1064 print("\r elapsed time ", "{0:5.0f}".format((ctime-atime)), "sec ", end="\r")
ulalume3@0 1065 ctime = clock()
ulalume3@0 1066 if ((ctime - dtime) > 10):
ulalume3@0 1067 print("\r elapsed time ", "{0:5.0f}".format((ctime-atime)), "sec ", end="\r")
ulalume3@0 1068 dtime = ctime
ulalume3@0 1069
ulalume3@0 1070 if nRotO > 0: RotO = RotO0 + iRotO*dRotO/nRotO
ulalume3@0 1071 if nRetO > 0: RetO = RetO0 + iRetO*dRetO/nRetO
ulalume3@0 1072 if nDiO > 0: DiO = DiO0 + iDiO*dDiO/nDiO
ulalume3@0 1073 if nRotC > 0: RotC = RotC0 + iRotC*dRotC/nRotC
ulalume3@0 1074 if nRetC > 0: RetC = RetC0 + iRetC*dRetC/nRetC
ulalume3@0 1075 if nDiC > 0: DiC = DiC0 + iDiC*dDiC/nDiC
ulalume3@0 1076 if nTP > 0: TP = TP0 + iTP*dTP/nTP
ulalume3@0 1077 if nTS > 0: TS = TS0 + iTS*dTS/nTS
ulalume3@0 1078 if nRP > 0: RP = RP0 + iRP*dRP/nRP
ulalume3@0 1079 if nRS > 0: RS = RS0 + iRS*dRS/nRS
ulalume3@0 1080 if nERaT > 0: ERaT = ERaT0 + iERaT*dERaT/nERaT
ulalume3@0 1081 if nRotaT > 0:RotaT= RotaT0+ iRotaT*dRotaT/nRotaT
ulalume3@0 1082 if nRetT > 0: RetT = RetT0 + iRetT*dRetT/nRetT
ulalume3@0 1083 if nERaR > 0: ERaR = ERaR0 + iERaR*dERaR/nERaR
ulalume3@0 1084 if nRotaR > 0:RotaR= RotaR0+ iRotaR*dRotaR/nRotaR
ulalume3@0 1085 if nRetR > 0: RetR = RetR0 + iRetR*dRetR/nRetR
ulalume3@0 1086
ulalume3@0 1087 #print("{0:5.2f}, {1:5.2f}, {2:5.2f}, {3:10d}".format(RotL, RotE, RotO, iN))
ulalume3@0 1088
ulalume3@0 1089 # receiver optics
ulalume3@0 1090 CosO = np.cos(np.deg2rad(RetO))
ulalume3@0 1091 SinO = np.sin(np.deg2rad(RetO))
ulalume3@0 1092 ZiO = (1. - DiO**2)**0.5
ulalume3@0 1093 WiO = (1. - ZiO*CosO)
ulalume3@0 1094 S2g = np.sin(np.deg2rad(2*RotO))
ulalume3@0 1095 C2g = np.cos(np.deg2rad(2*RotO))
ulalume3@0 1096 # calibrator
ulalume3@0 1097 CosC = np.cos(np.deg2rad(RetC))
ulalume3@0 1098 SinC = np.sin(np.deg2rad(RetC))
ulalume3@0 1099 ZiC = (1. - DiC**2)**0.5
ulalume3@0 1100 WiC = (1. - ZiC*CosC)
ulalume3@0 1101
ulalume3@0 1102 # analyser
volker@13 1103 #For POLLY_XTs
volker@13 1104 if(RS_RP_depend_on_TS_TP):
volker@13 1105 RS = 1 - TS
volker@13 1106 RP = 1 - TP
ulalume3@0 1107 TiT = 0.5 * (TP + TS)
ulalume3@0 1108 DiT = (TP-TS)/(TP+TS)
ulalume3@0 1109 ZiT = (1. - DiT**2)**0.5
ulalume3@0 1110 TiR = 0.5 * (RP + RS)
ulalume3@0 1111 DiR = (RP-RS)/(RP+RS)
ulalume3@0 1112 ZiR = (1. - DiR**2)**0.5
ulalume3@0 1113 CosT = np.cos(np.deg2rad(RetT))
ulalume3@0 1114 SinT = np.sin(np.deg2rad(RetT))
ulalume3@0 1115 CosR = np.cos(np.deg2rad(RetR))
ulalume3@0 1116 SinR = np.sin(np.deg2rad(RetR))
ulalume3@0 1117
ulalume3@0 1118 DaT = (1-ERaT)/(1+ERaT)
ulalume3@0 1119 DaR = (1-ERaR)/(1+ERaR)
ulalume3@0 1120 TaT = 0.5*(1+ERaT)
ulalume3@0 1121 TaR = 0.5*(1+ERaR)
ulalume3@0 1122
ulalume3@0 1123 S2aT = np.sin(np.deg2rad(h*2*RotaT))
ulalume3@0 1124 C2aT = np.cos(np.deg2rad(2*RotaT))
ulalume3@0 1125 S2aR = np.sin(np.deg2rad(h*2*RotaR))
ulalume3@0 1126 C2aR = np.cos(np.deg2rad(2*RotaR))
ulalume3@0 1127
ulalume3@0 1128 # Aanalyzer As before the PBS Eq. D.5
ulalume3@0 1129 ATP1 = (1+C2aT*DaT*DiT)
ulalume3@0 1130 ATP2 = Y*(DiT+C2aT*DaT)
ulalume3@0 1131 ATP3 = Y*S2aT*DaT*ZiT*CosT
ulalume3@0 1132 ATP4 = S2aT*DaT*ZiT*SinT
ulalume3@0 1133 ATP = np.array([ATP1,ATP2,ATP3,ATP4])
ulalume3@0 1134
ulalume3@0 1135 ARP1 = (1+C2aR*DaR*DiR)
ulalume3@0 1136 ARP2 = Y*(DiR+C2aR*DaR)
ulalume3@0 1137 ARP3 = Y*S2aR*DaR*ZiR*CosR
ulalume3@0 1138 ARP4 = S2aR*DaR*ZiR*SinR
ulalume3@0 1139 ARP = np.array([ARP1,ARP2,ARP3,ARP4])
ulalume3@0 1140
ulalume3@0 1141 TTa = TiT*TaT #*ATP1
ulalume3@0 1142 TRa = TiR*TaR #*ARP1
ulalume3@0 1143
ulalume3@0 1144 # ---- Calculate signals and correction parameters for diffeent locations and calibrators
ulalume3@0 1145 if LocC == 4: # Calibrator before the PBS
ulalume3@0 1146 #print("Calibrator location not implemented yet")
ulalume3@0 1147
ulalume3@0 1148 #S2ge = np.sin(np.deg2rad(2*RotO + h*2*RotC))
ulalume3@0 1149 #C2ge = np.cos(np.deg2rad(2*RotO + h*2*RotC))
ulalume3@0 1150 S2e = np.sin(np.deg2rad(h*2*RotC))
ulalume3@0 1151 C2e = np.cos(np.deg2rad(2*RotC))
ulalume3@0 1152 # rotated AinP by epsilon Eq. C.3
ulalume3@0 1153 ATP2e = C2e*ATP2 + S2e*ATP3
ulalume3@0 1154 ATP3e = C2e*ATP3 - S2e*ATP2
ulalume3@0 1155 ARP2e = C2e*ARP2 + S2e*ARP3
ulalume3@0 1156 ARP3e = C2e*ARP3 - S2e*ARP2
ulalume3@0 1157 ATPe = np.array([ATP1,ATP2e,ATP3e,ATP4])
ulalume3@0 1158 ARPe = np.array([ARP1,ARP2e,ARP3e,ARP4])
ulalume3@0 1159 # Stokes Input Vector before the polarising beam splitter Eq. E.31
ulalume3@0 1160 A = C2g*QinE - S2g*UinE
ulalume3@0 1161 B = S2g*QinE + C2g*UinE
ulalume3@0 1162 #C = (WiO*aCal*B + ZiO*SinO*(1-2*aCal)*VinE)
ulalume3@0 1163 Co = ZiO*SinO*VinE
ulalume3@0 1164 Ca = (WiO*B - 2*ZiO*SinO*VinE)
ulalume3@0 1165 #C = Co + aCal*Ca
ulalume3@0 1166 #IinP = (IinE + DiO*aCal*A)
ulalume3@0 1167 #QinP = (C2g*DiO*IinE + aCal*QinE - S2g*C)
ulalume3@0 1168 #UinP = (S2g*DiO*IinE - aCal*UinE + C2g*C)
ulalume3@0 1169 #VinP = (ZiO*SinO*aCal*B + ZiO*CosO*(1-2*aCal)*VinE)
ulalume3@0 1170 IinPo = IinE
ulalume3@0 1171 QinPo = (C2g*DiO*IinE - S2g*Co)
ulalume3@0 1172 UinPo = (S2g*DiO*IinE + C2g*Co)
ulalume3@0 1173 VinPo = ZiO*CosO*VinE
ulalume3@0 1174
ulalume3@0 1175 IinPa = DiO*A
ulalume3@0 1176 QinPa = QinE - S2g*Ca
ulalume3@0 1177 UinPa = -UinE + C2g*Ca
ulalume3@0 1178 VinPa = ZiO*(SinO*B - 2*CosO*VinE)
ulalume3@0 1179
ulalume3@0 1180 IinP = IinPo + aCal*IinPa
ulalume3@0 1181 QinP = QinPo + aCal*QinPa
ulalume3@0 1182 UinP = UinPo + aCal*UinPa
ulalume3@0 1183 VinP = VinPo + aCal*VinPa
ulalume3@0 1184 # Stokes Input Vector before the polarising beam splitter rotated by epsilon Eq. C.3
ulalume3@0 1185 #QinPe = C2e*QinP + S2e*UinP
ulalume3@0 1186 #UinPe = C2e*UinP - S2e*QinP
ulalume3@0 1187 QinPoe = C2e*QinPo + S2e*UinPo
ulalume3@0 1188 UinPoe = C2e*UinPo - S2e*QinPo
ulalume3@0 1189 QinPae = C2e*QinPa + S2e*UinPa
ulalume3@0 1190 UinPae = C2e*UinPa - S2e*QinPa
ulalume3@0 1191 QinPe = C2e*QinP + S2e*UinP
ulalume3@0 1192 UinPe = C2e*UinP - S2e*QinP
ulalume3@0 1193
ulalume3@0 1194 # Calibration signals and Calibration correction K from measurements with LDRCal / aCal
ulalume3@0 1195 if (TypeC == 2) or (TypeC == 1): # rotator calibration Eq. C.4
ulalume3@0 1196 # parameters for calibration with aCal
ulalume3@0 1197 AT = ATP1*IinP + h*ATP4*VinP
ulalume3@0 1198 BT = ATP3e*QinP - h*ATP2e*UinP
ulalume3@0 1199 AR = ARP1*IinP + h*ARP4*VinP
ulalume3@0 1200 BR = ARP3e*QinP - h*ARP2e*UinP
ulalume3@0 1201 # Correction paremeters for normal measurements; they are independent of LDR
ulalume3@0 1202 if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out
ulalume3@0 1203 IS1 = np.array([IinPo,QinPo,UinPo,VinPo])
ulalume3@0 1204 IS2 = np.array([IinPa,QinPa,UinPa,VinPa])
ulalume3@0 1205 GT = np.dot(ATP,IS1)
ulalume3@0 1206 GR = np.dot(ARP,IS1)
ulalume3@0 1207 HT = np.dot(ATP,IS2)
ulalume3@0 1208 HR = np.dot(ARP,IS2)
ulalume3@0 1209 else:
ulalume3@0 1210 IS1 = np.array([IinPo,QinPo,UinPo,VinPo])
ulalume3@0 1211 IS2 = np.array([IinPa,QinPa,UinPa,VinPa])
ulalume3@0 1212 GT = np.dot(ATPe,IS1)
ulalume3@0 1213 GR = np.dot(ARPe,IS1)
ulalume3@0 1214 HT = np.dot(ATPe,IS2)
ulalume3@0 1215 HR = np.dot(ARPe,IS2)
ulalume3@0 1216 elif (TypeC == 3) or (TypeC == 4): # linear polariser calibration Eq. C.5
ulalume3@0 1217 # parameters for calibration with aCal
ulalume3@0 1218 AT = ATP1*IinP + ATP3e*UinPe + ZiC*CosC*(ATP2e*QinPe + ATP4*VinP)
ulalume3@0 1219 BT = DiC*(ATP1*UinPe + ATP3e*IinP) - ZiC*SinC*(ATP2e*VinP - ATP4*QinPe)
ulalume3@0 1220 AR = ARP1*IinP + ARP3e*UinPe + ZiC*CosC*(ARP2e*QinPe + ARP4*VinP)
ulalume3@0 1221 BR = DiC*(ARP1*UinPe + ARP3e*IinP) - ZiC*SinC*(ARP2e*VinP - ARP4*QinPe)
ulalume3@0 1222 # Correction paremeters for normal measurements; they are independent of LDR
ulalume3@0 1223 if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out
ulalume3@0 1224 IS1 = np.array([IinPo,QinPo,UinPo,VinPo])
ulalume3@0 1225 IS2 = np.array([IinPa,QinPa,UinPa,VinPa])
ulalume3@0 1226 GT = np.dot(ATP,IS1)
ulalume3@0 1227 GR = np.dot(ARP,IS1)
ulalume3@0 1228 HT = np.dot(ATP,IS2)
ulalume3@0 1229 HR = np.dot(ARP,IS2)
ulalume3@0 1230 else:
ulalume3@0 1231 IS1e = np.array([IinPo+DiC*QinPoe,DiC*IinPo+QinPoe,ZiC*(CosC*UinPoe+SinC*VinPo),-ZiC*(SinC*UinPoe-CosC*VinPo)])
ulalume3@0 1232 IS2e = np.array([IinPa+DiC*QinPae,DiC*IinPa+QinPae,ZiC*(CosC*UinPae+SinC*VinPa),-ZiC*(SinC*UinPae-CosC*VinPa)])
ulalume3@0 1233 GT = np.dot(ATPe,IS1e)
ulalume3@0 1234 GR = np.dot(ARPe,IS1e)
ulalume3@0 1235 HT = np.dot(ATPe,IS2e)
ulalume3@0 1236 HR = np.dot(ARPe,IS2e)
ulalume3@0 1237 elif (TypeC == 6): # diattenuator calibration +-22.5° rotated_diattenuator_X22x5deg.odt
ulalume3@0 1238 # parameters for calibration with aCal
ulalume3@0 1239 AT = ATP1*IinP + sqr05*DiC*(ATP1*QinPe + ATP2e*IinP) + (1-0.5*WiC)*(ATP2e*QinPe + ATP3e*UinPe) + ZiC*(sqr05*SinC*(ATP3e*VinP-ATP4*UinPe) + ATP4*CosC*VinP)
ulalume3@0 1240 BT = sqr05*DiC*(ATP1*UinPe + ATP3e*IinP) + 0.5*WiC*(ATP2e*UinPe + ATP3e*QinPe) - sqr05*ZiC*SinC*(ATP2e*VinP - ATP4*QinPe)
ulalume3@0 1241 AR = ARP1*IinP + sqr05*DiC*(ARP1*QinPe + ARP2e*IinP) + (1-0.5*WiC)*(ARP2e*QinPe + ARP3e*UinPe) + ZiC*(sqr05*SinC*(ARP3e*VinP-ARP4*UinPe) + ARP4*CosC*VinP)
ulalume3@0 1242 BR = sqr05*DiC*(ARP1*UinPe + ARP3e*IinP) + 0.5*WiC*(ARP2e*UinPe + ARP3e*QinPe) - sqr05*ZiC*SinC*(ARP2e*VinP - ARP4*QinPe)
ulalume3@0 1243 # Correction paremeters for normal measurements; they are independent of LDR
ulalume3@0 1244 if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out
ulalume3@0 1245 IS1 = np.array([IinPo,QinPo,UinPo,VinPo])
ulalume3@0 1246 IS2 = np.array([IinPa,QinPa,UinPa,VinPa])
ulalume3@0 1247 GT = np.dot(ATP,IS1)
ulalume3@0 1248 GR = np.dot(ARP,IS1)
ulalume3@0 1249 HT = np.dot(ATP,IS2)
ulalume3@0 1250 HR = np.dot(ARP,IS2)
ulalume3@0 1251 else:
ulalume3@0 1252 IS1e = np.array([IinPo+DiC*QinPoe,DiC*IinPo+QinPoe,ZiC*(CosC*UinPoe+SinC*VinPo),-ZiC*(SinC*UinPoe-CosC*VinPo)])
ulalume3@0 1253 IS2e = np.array([IinPa+DiC*QinPae,DiC*IinPa+QinPae,ZiC*(CosC*UinPae+SinC*VinPa),-ZiC*(SinC*UinPae-CosC*VinPa)])
ulalume3@0 1254 GT = np.dot(ATPe,IS1e)
ulalume3@0 1255 GR = np.dot(ARPe,IS1e)
ulalume3@0 1256 HT = np.dot(ATPe,IS2e)
ulalume3@0 1257 HR = np.dot(ARPe,IS2e)
ulalume3@0 1258 else:
ulalume3@0 1259 print("Calibrator not implemented yet")
ulalume3@0 1260 sys.exit()
ulalume3@0 1261
ulalume3@0 1262 elif LocC == 3: # C before receiver optics Eq.57
ulalume3@0 1263
ulalume3@0 1264 #S2ge = np.sin(np.deg2rad(2*RotO - 2*RotC))
ulalume3@0 1265 #C2ge = np.cos(np.deg2rad(2*RotO - 2*RotC))
ulalume3@0 1266 S2e = np.sin(np.deg2rad(2*RotC))
ulalume3@0 1267 C2e = np.cos(np.deg2rad(2*RotC))
ulalume3@0 1268
ulalume3@0 1269 # AS with C before the receiver optics (see document rotated_diattenuator_X22x5deg.odt)
ulalume3@0 1270 AF1 = np.array([1,C2g*DiO,S2g*DiO,0])
ulalume3@0 1271 AF2 = np.array([C2g*DiO,1-S2g**2*WiO,S2g*C2g*WiO,-S2g*ZiO*SinO])
ulalume3@0 1272 AF3 = np.array([S2g*DiO, S2g*C2g*WiO, 1-C2g**2*WiO, C2g*ZiO*SinO])
ulalume3@0 1273 AF4 = np.array([0, S2g*SinO, -C2g*SinO, CosO])
ulalume3@0 1274
ulalume3@0 1275 ATF = (ATP1*AF1+ATP2*AF2+ATP3*AF3+ATP4*AF4)
ulalume3@0 1276 ARF = (ARP1*AF1+ARP2*AF2+ARP3*AF3+ARP4*AF4)
ulalume3@0 1277 ATF1 = ATF[0]
ulalume3@0 1278 ATF2 = ATF[1]
ulalume3@0 1279 ATF3 = ATF[2]
ulalume3@0 1280 ATF4 = ATF[3]
ulalume3@0 1281 ARF1 = ARF[0]
ulalume3@0 1282 ARF2 = ARF[1]
ulalume3@0 1283 ARF3 = ARF[2]
ulalume3@0 1284 ARF4 = ARF[3]
ulalume3@0 1285
ulalume3@0 1286 # rotated AinF by epsilon
ulalume3@0 1287 ATF2e = C2e*ATF[1] + S2e*ATF[2]
ulalume3@0 1288 ATF3e = C2e*ATF[2] - S2e*ATF[1]
ulalume3@0 1289 ARF2e = C2e*ARF[1] + S2e*ARF[2]
ulalume3@0 1290 ARF3e = C2e*ARF[2] - S2e*ARF[1]
ulalume3@0 1291
ulalume3@0 1292 ATFe = np.array([ATF1,ATF2e,ATF3e,ATF4])
ulalume3@0 1293 ARFe = np.array([ARF1,ARF2e,ARF3e,ARF4])
ulalume3@0 1294
ulalume3@0 1295 QinEe = C2e*QinE + S2e*UinE
ulalume3@0 1296 UinEe = C2e*UinE - S2e*QinE
ulalume3@0 1297
ulalume3@0 1298 # Stokes Input Vector before receiver optics Eq. E.19 (after atmosphere F)
ulalume3@0 1299 IinF = IinE
ulalume3@0 1300 QinF = aCal*QinE
ulalume3@0 1301 UinF = -aCal*UinE
ulalume3@0 1302 VinF = (1.-2.*aCal)*VinE
ulalume3@0 1303
ulalume3@0 1304 IinFo = IinE
ulalume3@0 1305 QinFo = 0.
ulalume3@0 1306 UinFo = 0.
ulalume3@0 1307 VinFo = VinE
ulalume3@0 1308
ulalume3@0 1309 IinFa = 0.
ulalume3@0 1310 QinFa = QinE
ulalume3@0 1311 UinFa = -UinE
ulalume3@0 1312 VinFa = -2.*VinE
ulalume3@0 1313
ulalume3@0 1314 # Stokes Input Vector before receiver optics rotated by epsilon Eq. C.3
ulalume3@0 1315 QinFe = C2e*QinF + S2e*UinF
ulalume3@0 1316 UinFe = C2e*UinF - S2e*QinF
ulalume3@0 1317 QinFoe = C2e*QinFo + S2e*UinFo
ulalume3@0 1318 UinFoe = C2e*UinFo - S2e*QinFo
ulalume3@0 1319 QinFae = C2e*QinFa + S2e*UinFa
ulalume3@0 1320 UinFae = C2e*UinFa - S2e*QinFa
ulalume3@0 1321
ulalume3@0 1322 # Calibration signals and Calibration correction K from measurements with LDRCal / aCal
ulalume3@0 1323 if (TypeC == 2) or (TypeC == 1): # rotator calibration Eq. C.4
ulalume3@0 1324 AT = ATF1*IinF + ATF4*h*VinF
ulalume3@0 1325 BT = ATF3e*QinF - ATF2e*h*UinF
ulalume3@0 1326 AR = ARF1*IinF + ARF4*h*VinF
ulalume3@0 1327 BR = ARF3e*QinF - ARF2e*h*UinF
ulalume3@0 1328
ulalume3@0 1329 # Correction paremeters for normal measurements; they are independent of LDR
ulalume3@0 1330 if (not RotationErrorEpsilonForNormalMeasurements):
ulalume3@0 1331 GT = ATF1*IinE + ATF4*VinE
ulalume3@0 1332 GR = ARF1*IinE + ARF4*VinE
ulalume3@0 1333 HT = ATF2*QinE - ATF3*UinE - ATF4*2*VinE
ulalume3@0 1334 HR = ARF2*QinE - ARF3*UinE - ARF4*2*VinE
ulalume3@0 1335 else:
ulalume3@0 1336 GT = ATF1*IinE + ATF4*h*VinE
ulalume3@0 1337 GR = ARF1*IinE + ARF4*h*VinE
ulalume3@0 1338 HT = ATF2e*QinE - ATF3e*h*UinE - ATF4*h*2*VinE
ulalume3@0 1339 HR = ARF2e*QinE - ARF3e*h*UinE - ARF4*h*2*VinE
ulalume3@0 1340
ulalume3@0 1341 elif (TypeC == 3) or (TypeC == 4): # linear polariser calibration Eq. C.5
ulalume3@0 1342 # p = +45°, m = -45°
ulalume3@0 1343 IF1e = np.array([IinF, ZiC*CosC*QinFe, UinFe, ZiC*CosC*VinF])
ulalume3@0 1344 IF2e = np.array([DiC*UinFe, -ZiC*SinC*VinF, DiC*IinF, ZiC*SinC*QinFe])
ulalume3@0 1345
ulalume3@0 1346 AT = np.dot(ATFe,IF1e)
ulalume3@0 1347 AR = np.dot(ARFe,IF1e)
ulalume3@0 1348 BT = np.dot(ATFe,IF2e)
ulalume3@0 1349 BR = np.dot(ARFe,IF2e)
ulalume3@0 1350
ulalume3@0 1351 # Correction paremeters for normal measurements; they are independent of LDR --- the same as for TypeC = 6
ulalume3@0 1352 if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out
ulalume3@0 1353 IS1 = np.array([IinE,0,0,VinE])
ulalume3@0 1354 IS2 = np.array([0,QinE,-UinE,-2*VinE])
ulalume3@0 1355
ulalume3@0 1356 GT = np.dot(ATF,IS1)
ulalume3@0 1357 GR = np.dot(ARF,IS1)
ulalume3@0 1358 HT = np.dot(ATF,IS2)
ulalume3@0 1359 HR = np.dot(ARF,IS2)
ulalume3@0 1360 else:
ulalume3@0 1361 IS1e = np.array([IinFo+DiC*QinFoe,DiC*IinFo+QinFoe,ZiC*(CosC*UinFoe+SinC*VinFo),-ZiC*(SinC*UinFoe-CosC*VinFo)])
ulalume3@0 1362 IS2e = np.array([IinFa+DiC*QinFae,DiC*IinFa+QinFae,ZiC*(CosC*UinFae+SinC*VinFa),-ZiC*(SinC*UinFae-CosC*VinFa)])
ulalume3@0 1363 GT = np.dot(ATFe,IS1e)
ulalume3@0 1364 GR = np.dot(ARFe,IS1e)
ulalume3@0 1365 HT = np.dot(ATFe,IS2e)
ulalume3@0 1366 HR = np.dot(ARFe,IS2e)
ulalume3@0 1367
ulalume3@0 1368 elif (TypeC == 6): # diattenuator calibration +-22.5° rotated_diattenuator_X22x5deg.odt
ulalume3@0 1369 # p = +22.5°, m = -22.5°
ulalume3@0 1370 IF1e = np.array([IinF+sqr05*DiC*QinFe, sqr05*DiC*IinF+(1-0.5*WiC)*QinFe, (1-0.5*WiC)*UinFe+sqr05*ZiC*SinC*VinF, -sqr05*ZiC*SinC*UinFe+ZiC*CosC*VinF])
ulalume3@0 1371 IF2e = np.array([sqr05*DiC*UinFe, 0.5*WiC*UinFe-sqr05*ZiC*SinC*VinF, sqr05*DiC*IinF+0.5*WiC*QinFe, sqr05*ZiC*SinC*QinFe])
ulalume3@0 1372
ulalume3@0 1373 AT = np.dot(ATFe,IF1e)
ulalume3@0 1374 AR = np.dot(ARFe,IF1e)
ulalume3@0 1375 BT = np.dot(ATFe,IF2e)
ulalume3@0 1376 BR = np.dot(ARFe,IF2e)
ulalume3@0 1377
ulalume3@0 1378 # Correction paremeters for normal measurements; they are independent of LDR
ulalume3@0 1379 if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out
ulalume3@0 1380 #IS1 = np.array([IinE,0,0,VinE])
ulalume3@0 1381 #IS2 = np.array([0,QinE,-UinE,-2*VinE])
ulalume3@0 1382 IS1 = np.array([IinFo,0,0,VinFo])
ulalume3@0 1383 IS2 = np.array([0,QinFa,UinFa,VinFa])
ulalume3@0 1384 GT = np.dot(ATF,IS1)
ulalume3@0 1385 GR = np.dot(ARF,IS1)
ulalume3@0 1386 HT = np.dot(ATF,IS2)
ulalume3@0 1387 HR = np.dot(ARF,IS2)
ulalume3@0 1388 else:
ulalume3@0 1389 #IS1e = np.array([IinE,DiC*IinE,ZiC*SinC*VinE,ZiC*CosC*VinE])
ulalume3@0 1390 #IS2e = np.array([DiC*QinEe,QinEe,-ZiC*(CosC*UinEe+2*SinC*VinE),ZiC*(SinC*UinEe-2*CosC*VinE)])
ulalume3@0 1391 IS1e = np.array([IinFo+DiC*QinFoe,DiC*IinFo+QinFoe,ZiC*(CosC*UinFoe+SinC*VinFo),-ZiC*(SinC*UinFoe-CosC*VinFo)])
ulalume3@0 1392 IS2e = np.array([IinFa+DiC*QinFae,DiC*IinFa+QinFae,ZiC*(CosC*UinFae+SinC*VinFa),-ZiC*(SinC*UinFae-CosC*VinFa)])
ulalume3@0 1393 GT = np.dot(ATFe,IS1e)
ulalume3@0 1394 GR = np.dot(ARFe,IS1e)
ulalume3@0 1395 HT = np.dot(ATFe,IS2e)
ulalume3@0 1396 HR = np.dot(ARFe,IS2e)
ulalume3@0 1397
ulalume3@0 1398
ulalume3@0 1399 else:
ulalume3@0 1400 print('Calibrator not implemented yet')
ulalume3@0 1401 sys.exit()
ulalume3@0 1402
ulalume3@0 1403 elif LocC == 2: # C behind emitter optics Eq.57
ulalume3@0 1404 #print("Calibrator location not implemented yet")
ulalume3@0 1405 S2e = np.sin(np.deg2rad(2*RotC))
ulalume3@0 1406 C2e = np.cos(np.deg2rad(2*RotC))
ulalume3@0 1407
ulalume3@0 1408 # AS with C before the receiver optics (see document rotated_diattenuator_X22x5deg.odt)
ulalume3@0 1409 AF1 = np.array([1,C2g*DiO,S2g*DiO,0])
ulalume3@0 1410 AF2 = np.array([C2g*DiO,1-S2g**2*WiO,S2g*C2g*WiO,-S2g*ZiO*SinO])
ulalume3@0 1411 AF3 = np.array([S2g*DiO, S2g*C2g*WiO, 1-C2g**2*WiO, C2g*ZiO*SinO])
ulalume3@0 1412 AF4 = np.array([0, S2g*SinO, -C2g*SinO, CosO])
ulalume3@0 1413
ulalume3@0 1414 ATF = (ATP1*AF1+ATP2*AF2+ATP3*AF3+ATP4*AF4)
ulalume3@0 1415 ARF = (ARP1*AF1+ARP2*AF2+ARP3*AF3+ARP4*AF4)
ulalume3@0 1416 ATF1 = ATF[0]
ulalume3@0 1417 ATF2 = ATF[1]
ulalume3@0 1418 ATF3 = ATF[2]
ulalume3@0 1419 ATF4 = ATF[3]
ulalume3@0 1420 ARF1 = ARF[0]
ulalume3@0 1421 ARF2 = ARF[1]
ulalume3@0 1422 ARF3 = ARF[2]
ulalume3@0 1423 ARF4 = ARF[3]
ulalume3@0 1424
ulalume3@0 1425 # AS with C behind the emitter --------------------------------------------
ulalume3@0 1426 # terms without aCal
ulalume3@0 1427 ATE1o, ARE1o = ATF1, ARF1
ulalume3@0 1428 ATE2o, ARE2o = 0., 0.
ulalume3@0 1429 ATE3o, ARE3o = 0., 0.
ulalume3@0 1430 ATE4o, ARE4o = ATF4, ARF4
ulalume3@0 1431 # terms with aCal
ulalume3@0 1432 ATE1a, ARE1a = 0. , 0.
ulalume3@0 1433 ATE2a, ARE2a = ATF2, ARF2
ulalume3@0 1434 ATE3a, ARE3a = -ATF3, -ARF3
ulalume3@0 1435 ATE4a, ARE4a = -2*ATF4, -2*ARF4
ulalume3@0 1436 # rotated AinEa by epsilon
ulalume3@0 1437 ATE2ae = C2e*ATF2 + S2e*ATF3
ulalume3@0 1438 ATE3ae = -S2e*ATF2 - C2e*ATF3
ulalume3@0 1439 ARE2ae = C2e*ARF2 + S2e*ARF3
ulalume3@0 1440 ARE3ae = -S2e*ARF2 - C2e*ARF3
ulalume3@0 1441
ulalume3@0 1442 ATE1 = ATE1o
ulalume3@0 1443 ATE2e = aCal*ATE2ae
ulalume3@0 1444 ATE3e = aCal*ATE3ae
ulalume3@0 1445 ATE4 = (1-2*aCal)*ATF4
ulalume3@0 1446 ARE1 = ARE1o
ulalume3@0 1447 ARE2e = aCal*ARE2ae
ulalume3@0 1448 ARE3e = aCal*ARE3ae
ulalume3@0 1449 ARE4 = (1-2*aCal)*ARF4
ulalume3@0 1450
ulalume3@0 1451 # rotated IinE
ulalume3@0 1452 QinEe = C2e*QinE + S2e*UinE
ulalume3@0 1453 UinEe = C2e*UinE - S2e*QinE
ulalume3@0 1454
ulalume3@0 1455 # --- Calibration signals and Calibration correction K from measurements with LDRCal / aCal
ulalume3@0 1456 if (TypeC == 2) or (TypeC == 1): # +++++++++ rotator calibration Eq. C.4
ulalume3@0 1457 AT = ATE1o*IinE + (ATE4o+aCal*ATE4a)*h*VinE
ulalume3@0 1458 BT = aCal * (ATE3ae*QinEe - ATE2ae*h*UinEe)
ulalume3@0 1459 AR = ARE1o*IinE + (ARE4o+aCal*ARE4a)*h*VinE
ulalume3@0 1460 BR = aCal * (ARE3ae*QinEe - ARE2ae*h*UinEe)
ulalume3@0 1461
ulalume3@0 1462 # Correction paremeters for normal measurements; they are independent of LDR
ulalume3@0 1463 if (not RotationErrorEpsilonForNormalMeasurements):
ulalume3@0 1464 # Stokes Input Vector before receiver optics Eq. E.19 (after atmosphere F)
ulalume3@0 1465 GT = ATE1o*IinE + ATE4o*h*VinE
ulalume3@0 1466 GR = ARE1o*IinE + ARE4o*h*VinE
ulalume3@0 1467 HT = ATE2a*QinE + ATE3a*h*UinEe + ATE4a*h*VinE
ulalume3@0 1468 HR = ARE2a*QinE + ARE3a*h*UinEe + ARE4a*h*VinE
ulalume3@0 1469 else:
ulalume3@0 1470 GT = ATE1o*IinE + ATE4o*h*VinE
ulalume3@0 1471 GR = ARE1o*IinE + ARE4o*h*VinE
ulalume3@0 1472 HT = ATE2ae*QinE + ATE3ae*h*UinEe + ATE4a*h*VinE
ulalume3@0 1473 HR = ARE2ae*QinE + ARE3ae*h*UinEe + ARE4a*h*VinE
ulalume3@0 1474
ulalume3@0 1475 elif (TypeC == 3) or (TypeC == 4): # +++++++++ linear polariser calibration Eq. C.5
ulalume3@0 1476 # p = +45°, m = -45°
ulalume3@0 1477 AT = ATE1*IinE + ZiC*CosC*(ATE2e*QinEe + ATE4*VinE) + ATE3e*UinEe
ulalume3@0 1478 BT = DiC*(ATE1*UinEe + ATE3e*IinE) + ZiC*SinC*(ATE4*QinEe - ATE2e*VinE)
ulalume3@0 1479 AR = ARE1*IinE + ZiC*CosC*(ARE2e*QinEe + ARE4*VinE) + ARE3e*UinEe
ulalume3@0 1480 BR = DiC*(ARE1*UinEe + ARE3e*IinE) + ZiC*SinC*(ARE4*QinEe - ARE2e*VinE)
ulalume3@0 1481
ulalume3@0 1482 # Correction paremeters for normal measurements; they are independent of LDR
ulalume3@0 1483 if (not RotationErrorEpsilonForNormalMeasurements):
ulalume3@0 1484 # Stokes Input Vector before receiver optics Eq. E.19 (after atmosphere F)
ulalume3@0 1485 GT = ATE1o*IinE + ATE4o*VinE
ulalume3@0 1486 GR = ARE1o*IinE + ARE4o*VinE
ulalume3@0 1487 HT = ATE2a*QinE + ATE3a*UinE + ATE4a*VinE
ulalume3@0 1488 HR = ARE2a*QinE + ARE3a*UinE + ARE4a*VinE
ulalume3@0 1489 else:
ulalume3@0 1490 D = IinE + DiC*QinEe
ulalume3@0 1491 A = DiC*IinE + QinEe
ulalume3@0 1492 B = ZiC*(CosC*UinEe + SinC*VinE)
ulalume3@0 1493 C = -ZiC*(SinC*UinEe - CosC*VinE)
ulalume3@0 1494 GT = ATE1o*D + ATE4o*C
ulalume3@0 1495 GR = ARE1o*D + ARE4o*C
ulalume3@0 1496 HT = ATE2a*A + ATE3a*B + ATE4a*C
ulalume3@0 1497 HR = ARE2a*A + ARE3a*B + ARE4a*C
ulalume3@0 1498
ulalume3@0 1499 elif (TypeC == 6): # real HWP calibration +-22.5° rotated_diattenuator_X22x5deg.odt
ulalume3@0 1500 # p = +22.5°, m = -22.5°
ulalume3@0 1501 IE1e = np.array([IinE+sqr05*DiC*QinEe, sqr05*DiC*IinE+(1-0.5*WiC)*QinEe, (1-0.5*WiC)*UinEe+sqr05*ZiC*SinC*VinE, -sqr05*ZiC*SinC*UinEe+ZiC*CosC*VinE])
ulalume3@0 1502 IE2e = np.array([sqr05*DiC*UinEe, 0.5*WiC*UinEe-sqr05*ZiC*SinC*VinE, sqr05*DiC*IinE+0.5*WiC*QinEe, sqr05*ZiC*SinC*QinEe])
ulalume3@0 1503 ATEe = np.array([ATE1,ATE2e,ATE3e,ATE4])
ulalume3@0 1504 AREe = np.array([ARE1,ARE2e,ARE3e,ARE4])
ulalume3@0 1505 AT = np.dot(ATEe,IE1e)
ulalume3@0 1506 AR = np.dot(AREe,IE1e)
ulalume3@0 1507 BT = np.dot(ATEe,IE2e)
ulalume3@0 1508 BR = np.dot(AREe,IE2e)
ulalume3@0 1509
ulalume3@0 1510 # Correction paremeters for normal measurements; they are independent of LDR
ulalume3@0 1511 if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out
ulalume3@0 1512 GT = ATE1o*IinE + ATE4o*VinE
ulalume3@0 1513 GR = ARE1o*IinE + ARE4o*VinE
ulalume3@0 1514 HT = ATE2a*QinE + ATE3a*UinE + ATE4a*VinE
ulalume3@0 1515 HR = ARE2a*QinE + ARE3a*UinE + ARE4a*VinE
ulalume3@0 1516 else:
ulalume3@0 1517 D = IinE + DiC*QinEe
ulalume3@0 1518 A = DiC*IinE + QinEe
ulalume3@0 1519 B = ZiC*(CosC*UinEe + SinC*VinE)
ulalume3@0 1520 C = -ZiC*(SinC*UinEe - CosC*VinE)
ulalume3@0 1521 GT = ATE1o*D + ATE4o*C
ulalume3@0 1522 GR = ARE1o*D + ARE4o*C
ulalume3@0 1523 HT = ATE2a*A + ATE3a*B + ATE4a*C
ulalume3@0 1524 HR = ARE2a*A + ARE3a*B + ARE4a*C
ulalume3@0 1525
ulalume3@0 1526 else:
ulalume3@0 1527 print('Calibrator not implemented yet')
ulalume3@0 1528 sys.exit()
ulalume3@0 1529
ulalume3@0 1530 # Calibration signals with aCal => Determination of the correction K of the real calibration factor
ulalume3@0 1531 IoutTp = TaT*TiT*TiO*TiE*(AT + BT)
ulalume3@0 1532 IoutTm = TaT*TiT*TiO*TiE*(AT - BT)
ulalume3@0 1533 IoutRp = TaR*TiR*TiO*TiE*(AR + BR)
ulalume3@0 1534 IoutRm = TaR*TiR*TiO*TiE*(AR - BR)
ulalume3@0 1535 # --- Results and Corrections; electronic etaR and etaT are assumed to be 1
ulalume3@0 1536 #Eta = TiR/TiT # Eta = Eta*/K Eq. 84
ulalume3@0 1537 Etapx = IoutRp/IoutTp
ulalume3@0 1538 Etamx = IoutRm/IoutTm
ulalume3@0 1539 Etax = (Etapx*Etamx)**0.5
ulalume3@0 1540 K = Etax / Eta0
ulalume3@0 1541 #print("{0:6.3f},{1:6.3f},{2:6.3f},{3:6.3f},{4:6.3f},{5:6.3f},{6:6.3f},{7:6.3f},{8:6.3f},{9:6.3f},{10:6.3f}".format(AT, BT, AR, BR, DiC, ZiC, RetO, TP, TS, Kp, Km))
ulalume3@0 1542 #print("{0:6.3f},{1:6.3f},{2:6.3f},{3:6.3f}".format(DiC, ZiC, Kp, Km))
ulalume3@0 1543
ulalume3@0 1544 # For comparison with Volkers Libreoffice Müller Matrix spreadsheet
ulalume3@0 1545 #Eta_test_p = (IoutRp/IoutTp)
ulalume3@0 1546 #Eta_test_m = (IoutRm/IoutTm)
ulalume3@0 1547 #Eta_test = (Eta_test_p*Eta_test_m)**0.5
ulalume3@0 1548
ulalume3@0 1549 # *************************************************************************
ulalume3@0 1550 iLDR = -1
ulalume3@0 1551 for LDRTrue in LDRrange:
ulalume3@0 1552 iLDR = iLDR + 1
ulalume3@0 1553 atrue = (1-LDRTrue)/(1+LDRTrue)
ulalume3@0 1554 # ----- Forward simulated signals and LDRsim with atrue; from input file
ulalume3@0 1555 It = TaT*TiT*TiO*TiE*(GT+atrue*HT) # TaT*TiT*TiC*TiO*IinL*(GT+atrue*HT)
ulalume3@0 1556 Ir = TaR*TiR*TiO*TiE*(GR+atrue*HR) # TaR*TiR*TiC*TiO*IinL*(GR+atrue*HR)
ulalume3@0 1557
ulalume3@0 1558 # LDRsim = 1/Eta*Ir/It # simulated LDR* with Y from input file
ulalume3@0 1559 LDRsim = Ir/It # simulated uncorrected LDR with Y from input file
ulalume3@0 1560 '''
ulalume3@0 1561 if Y == 1.:
ulalume3@0 1562 LDRsimx = LDRsim
ulalume3@0 1563 LDRsimx2 = LDRsim2
ulalume3@0 1564 else:
ulalume3@0 1565 LDRsimx = 1./LDRsim
ulalume3@0 1566 LDRsimx2 = 1./LDRsim2
ulalume3@0 1567 '''
ulalume3@0 1568 # ----- Backward correction
ulalume3@0 1569 # Corrected LDRCorr from forward simulated LDRsim (atrue) with assumed true G0,H0,K0
ulalume3@0 1570 LDRCorr = (LDRsim*K0/Etax*(GT0+HT0)-(GR0+HR0))/((GR0-HR0)-LDRsim*K0/Etax*(GT0-HT0))
ulalume3@0 1571
ulalume3@0 1572 # -- F11corr from It and Ir and calibration EtaX
volker@11 1573 Text1 = "!!! EXPERIMENTAL !!! F11corr from It and Ir with calibration EtaX: x-axis: F11corr(LDRtrue) / F11corr(LDRtrue = 0.004) - 1"
ulalume3@0 1574 F11corr = 1/(TiO*TiE)*((HR0*Etax/K0*It/TTa-HT0*Ir/TRa)/(HR0*GT0-HT0*GR0)) # IL = 1 Eq.(64)
ulalume3@0 1575
ulalume3@0 1576 #Text1 = "F11corr from It and Ir without corrections but with calibration EtaX: x-axis: F11corr(LDRtrue) devided by F11corr(LDRtrue = 0.004)"
ulalume3@0 1577 #F11corr = 0.5/(TiO*TiE)*(Etax*It/TTa+Ir/TRa) # IL = 1 Eq.(64)
ulalume3@0 1578
ulalume3@0 1579 # -- It from It only with atrue without corrections - for BERTHA (and PollyXTs)
ulalume3@0 1580 #Text1 = " x-axis: IT(LDRtrue) / IT(LDRtrue = 0.004) - 1"
ulalume3@0 1581 #F11corr = It/(TaT*TiT*TiO*TiE) #/(TaT*TiT*TiO*TiE*(GT0+atrue*HT0))
ulalume3@0 1582 # !!! see below line 1673ff
ulalume3@0 1583
ulalume3@0 1584 aF11corr[iLDR,iN] = F11corr
ulalume3@0 1585 aA[iLDR,iN] = LDRCorr
ulalume3@0 1586
ulalume3@0 1587 aX[0,iN] = GR
ulalume3@0 1588 aX[1,iN] = GT
ulalume3@0 1589 aX[2,iN] = HR
ulalume3@0 1590 aX[3,iN] = HT
ulalume3@0 1591 aX[4,iN] = K
ulalume3@0 1592
ulalume3@0 1593 aLDRCal[iN] = iLDRCal
ulalume3@0 1594 aERaT[iN] = iERaT
ulalume3@0 1595 aERaR[iN] = iERaR
ulalume3@0 1596 aRotaT[iN] = iRotaT
ulalume3@0 1597 aRotaR[iN] = iRotaR
ulalume3@0 1598 aRetT[iN] = iRetT
ulalume3@0 1599 aRetR[iN] = iRetR
ulalume3@0 1600
ulalume3@0 1601 aRotL[iN] = iRotL
ulalume3@0 1602 aRotE[iN] = iRotE
ulalume3@0 1603 aRetE[iN] = iRetE
ulalume3@0 1604 aRotO[iN] = iRotO
ulalume3@0 1605 aRetO[iN] = iRetO
ulalume3@0 1606 aRotC[iN] = iRotC
ulalume3@0 1607 aRetC[iN] = iRetC
ulalume3@0 1608 aDiO[iN] = iDiO
ulalume3@0 1609 aDiE[iN] = iDiE
ulalume3@0 1610 aDiC[iN] = iDiC
ulalume3@0 1611 aTP[iN] = iTP
ulalume3@0 1612 aTS[iN] = iTS
ulalume3@0 1613 aRP[iN] = iRP
ulalume3@0 1614 aRS[iN] = iRS
ulalume3@0 1615
ulalume3@0 1616 # --- END loop
ulalume3@0 1617 btime = clock()
ulalume3@0 1618 print("\r done in ", "{0:5.0f}".format(btime-atime), "sec") #, end="\r")
ulalume3@0 1619
ulalume3@0 1620 # --- Plot -----------------------------------------------------------------
volker@11 1621 if (sns_loaded):
volker@11 1622 sns.set_style("whitegrid")
volker@11 1623 sns.set_palette("bright", 6)
ulalume3@0 1624
ulalume3@0 1625 '''
ulalume3@0 1626 fig2 = plt.figure()
ulalume3@0 1627 plt.plot(aA[2,:],'b.')
ulalume3@0 1628 plt.plot(aA[3,:],'r.')
ulalume3@0 1629 plt.plot(aA[4,:],'g.')
ulalume3@0 1630 #plt.plot(aA[6,:],'c.')
ulalume3@0 1631 plt.show
ulalume3@0 1632 '''
ulalume3@0 1633 # Plot LDR
ulalume3@0 1634 def PlotSubHist(aVar, aX, X0, daX, iaX, naX):
ulalume3@0 1635 fig, ax = plt.subplots(nrows=1, ncols=5, sharex=True, sharey=True, figsize=(25, 2))
ulalume3@0 1636 iLDR = -1
ulalume3@0 1637 for LDRTrue in LDRrange:
ulalume3@0 1638 iLDR = iLDR + 1
ulalume3@0 1639
ulalume3@0 1640 LDRmin[iLDR] = np.min(aA[iLDR,:])
ulalume3@0 1641 LDRmax[iLDR] = np.max(aA[iLDR,:])
ulalume3@0 1642 Rmin = LDRmin[iLDR] * 0.995 # np.min(aA[iLDR,:]) * 0.995
ulalume3@0 1643 Rmax = LDRmax[iLDR] * 1.005 # np.max(aA[iLDR,:]) * 1.005
ulalume3@0 1644
ulalume3@0 1645 #plt.subplot(5,2,iLDR+1)
ulalume3@0 1646 plt.subplot(1,5,iLDR+1)
ulalume3@0 1647 (n, bins, patches) = plt.hist(aA[iLDR,:],
ulalume3@0 1648 bins=100, log=False,
ulalume3@0 1649 range=[Rmin, Rmax],
ulalume3@0 1650 alpha=0.5, normed=False, color = '0.5', histtype='stepfilled')
ulalume3@0 1651
ulalume3@0 1652 for iaX in range(-naX,naX+1):
ulalume3@0 1653 plt.hist(aA[iLDR,aX == iaX],
ulalume3@0 1654 range=[Rmin, Rmax],
ulalume3@0 1655 bins=100, log=False, alpha=0.3, normed=False, histtype='stepfilled', label = str(round(X0 + iaX*daX/naX,5)))
ulalume3@0 1656
ulalume3@0 1657 if (iLDR == 2): plt.legend()
ulalume3@0 1658
ulalume3@0 1659 plt.tick_params(axis='both', labelsize=9)
ulalume3@0 1660 plt.plot([LDRTrue, LDRTrue], [0, np.max(n)], 'r-', lw=2)
ulalume3@0 1661
ulalume3@0 1662 #plt.title(LID + ' ' + aVar, fontsize=18)
ulalume3@0 1663 #plt.ylabel('frequency', fontsize=10)
ulalume3@0 1664 #plt.xlabel('LDRcorr', fontsize=10)
ulalume3@0 1665 #fig.tight_layout()
ulalume3@0 1666 fig.suptitle(LID + ' ' + str(Type[TypeC]) + ' ' + str(Loc[LocC]) + ' - ' + aVar, fontsize=14, y=1.05)
ulalume3@0 1667 #plt.show()
ulalume3@0 1668 #fig.savefig(LID + '_' + aVar + '.png', dpi=150, bbox_inches='tight', pad_inches=0)
ulalume3@0 1669 #plt.close
ulalume3@0 1670 return
ulalume3@0 1671
ulalume3@0 1672 if (nRotL > 0): PlotSubHist("RotL", aRotL, RotL0, dRotL, iRotL, nRotL)
ulalume3@0 1673 if (nRetE > 0): PlotSubHist("RetE", aRetE, RetE0, dRetE, iRetE, nRetE)
ulalume3@0 1674 if (nRotE > 0): PlotSubHist("RotE", aRotE, RotE0, dRotE, iRotE, nRotE)
ulalume3@0 1675 if (nDiE > 0): PlotSubHist("DiE", aDiE, DiE0, dDiE, iDiE, nDiE)
ulalume3@0 1676 if (nRetO > 0): PlotSubHist("RetO", aRetO, RetO0, dRetO, iRetO, nRetO)
ulalume3@0 1677 if (nRotO > 0): PlotSubHist("RotO", aRotO, RotO0, dRotO, iRotO, nRotO)
ulalume3@0 1678 if (nDiO > 0): PlotSubHist("DiO", aDiO, DiO0, dDiO, iDiO, nDiO)
ulalume3@0 1679 if (nDiC > 0): PlotSubHist("DiC", aDiC, DiC0, dDiC, iDiC, nDiC)
ulalume3@0 1680 if (nRotC > 0): PlotSubHist("RotC", aRotC, RotC0, dRotC, iRotC, nRotC)
ulalume3@0 1681 if (nRetC > 0): PlotSubHist("RetC", aRetC, RetC0, dRetC, iRetC, nRetC)
ulalume3@0 1682 if (nTP > 0): PlotSubHist("TP", aTP, TP0, dTP, iTP, nTP)
ulalume3@0 1683 if (nTS > 0): PlotSubHist("TS", aTS, TS0, dTS, iTS, nTS)
ulalume3@0 1684 if (nRP > 0): PlotSubHist("RP", aRP, RP0, dRP, iRP, nRP)
ulalume3@0 1685 if (nRS > 0): PlotSubHist("RS", aRS, RS0, dRS, iRS, nRS)
ulalume3@0 1686 if (nRetT > 0): PlotSubHist("RetT", aRetT, RetT0, dRetT, iRetT, nRetT)
ulalume3@0 1687 if (nRetR > 0): PlotSubHist("RetR", aRetR, RetR0, dRetR, iRetR, nRetR)
ulalume3@0 1688 if (nERaT > 0): PlotSubHist("ERaT", aERaT, ERaT0, dERaT, iERaT, nERaT)
ulalume3@0 1689 if (nERaR > 0): PlotSubHist("ERaR", aERaR, ERaR0, dERaR, iERaR, nERaR)
ulalume3@0 1690 if (nRotaT > 0): PlotSubHist("RotaT", aRotaT, RotaT0, dRotaT, iRotaT, nRotaT)
ulalume3@0 1691 if (nRotaR > 0): PlotSubHist("RotaR", aRotaR, RotaR0, dRotaR, iRotaR, nRotaR)
ulalume3@0 1692 if (nLDRCal > 0): PlotSubHist("LDRCal", aLDRCal, LDRCal0, dLDRCal, iLDRCal, nLDRCal)
ulalume3@0 1693
ulalume3@0 1694 plt.show()
ulalume3@0 1695 plt.close
ulalume3@0 1696
ulalume3@0 1697 print()
ulalume3@0 1698 #print("IT(LDRtrue) devided by IT(LDRtrue = 0.004)")
volker@11 1699 print(" ############################################################################## ")
ulalume3@0 1700 print(Text1)
ulalume3@0 1701 print()
ulalume3@0 1702
ulalume3@0 1703 iLDR = 5
ulalume3@0 1704 for LDRTrue in LDRrange:
ulalume3@0 1705 iLDR = iLDR - 1
ulalume3@0 1706 aF11corr[iLDR,:] = aF11corr[iLDR,:] / aF11corr[0,:] - 1.0
ulalume3@0 1707
ulalume3@0 1708 # Plot F11
ulalume3@0 1709 def PlotSubHistF11(aVar, aX, X0, daX, iaX, naX):
ulalume3@0 1710 fig, ax = plt.subplots(nrows=1, ncols=5, sharex=True, sharey=True, figsize=(25, 2))
ulalume3@0 1711 iLDR = -1
ulalume3@0 1712 for LDRTrue in LDRrange:
ulalume3@0 1713 iLDR = iLDR + 1
ulalume3@0 1714
ulalume3@0 1715 '''
ulalume3@0 1716 F11min[iLDR] = np.min(aF11corr[iLDR,:])
ulalume3@0 1717 F11max[iLDR] = np.max(aF11corr[iLDR,:])
ulalume3@0 1718 Rmin = F11min[iLDR] * 0.995 # np.min(aA[iLDR,:]) * 0.995
ulalume3@0 1719 Rmax = F11max[iLDR] * 1.005 # np.max(aA[iLDR,:]) * 1.005
ulalume3@0 1720 '''
ulalume3@0 1721 #Rmin = 0.8
ulalume3@0 1722 #Rmax = 1.2
ulalume3@0 1723
ulalume3@0 1724 #plt.subplot(5,2,iLDR+1)
ulalume3@0 1725 plt.subplot(1,5,iLDR+1)
ulalume3@0 1726 (n, bins, patches) = plt.hist(aF11corr[iLDR,:],
ulalume3@0 1727 bins=100, log=False,
ulalume3@0 1728 alpha=0.5, normed=False, color = '0.5', histtype='stepfilled')
ulalume3@0 1729
ulalume3@0 1730 for iaX in range(-naX,naX+1):
ulalume3@0 1731 plt.hist(aF11corr[iLDR,aX == iaX],
ulalume3@0 1732 bins=100, log=False, alpha=0.3, normed=False, histtype='stepfilled', label = str(round(X0 + iaX*daX/naX,5)))
ulalume3@0 1733
ulalume3@0 1734 if (iLDR == 2): plt.legend()
ulalume3@0 1735
ulalume3@0 1736 plt.tick_params(axis='both', labelsize=9)
ulalume3@0 1737 #plt.plot([LDRTrue, LDRTrue], [0, np.max(n)], 'r-', lw=2)
ulalume3@0 1738
ulalume3@0 1739 #plt.title(LID + ' ' + aVar, fontsize=18)
ulalume3@0 1740 #plt.ylabel('frequency', fontsize=10)
ulalume3@0 1741 #plt.xlabel('LDRcorr', fontsize=10)
ulalume3@0 1742 #fig.tight_layout()
ulalume3@0 1743 fig.suptitle(LID + ' ' + str(Type[TypeC]) + ' ' + str(Loc[LocC]) + ' - ' + aVar, fontsize=14, y=1.05)
ulalume3@0 1744 #plt.show()
ulalume3@0 1745 #fig.savefig(LID + '_' + aVar + '.png', dpi=150, bbox_inches='tight', pad_inches=0)
ulalume3@0 1746 #plt.close
ulalume3@0 1747 return
ulalume3@0 1748
ulalume3@0 1749 if (nRotL > 0): PlotSubHistF11("RotL", aRotL, RotL0, dRotL, iRotL, nRotL)
ulalume3@0 1750 if (nRetE > 0): PlotSubHistF11("RetE", aRetE, RetE0, dRetE, iRetE, nRetE)
ulalume3@0 1751 if (nRotE > 0): PlotSubHistF11("RotE", aRotE, RotE0, dRotE, iRotE, nRotE)
ulalume3@0 1752 if (nDiE > 0): PlotSubHistF11("DiE", aDiE, DiE0, dDiE, iDiE, nDiE)
ulalume3@0 1753 if (nRetO > 0): PlotSubHistF11("RetO", aRetO, RetO0, dRetO, iRetO, nRetO)
ulalume3@0 1754 if (nRotO > 0): PlotSubHistF11("RotO", aRotO, RotO0, dRotO, iRotO, nRotO)
ulalume3@0 1755 if (nDiO > 0): PlotSubHistF11("DiO", aDiO, DiO0, dDiO, iDiO, nDiO)
ulalume3@0 1756 if (nDiC > 0): PlotSubHistF11("DiC", aDiC, DiC0, dDiC, iDiC, nDiC)
ulalume3@0 1757 if (nRotC > 0): PlotSubHistF11("RotC", aRotC, RotC0, dRotC, iRotC, nRotC)
ulalume3@0 1758 if (nRetC > 0): PlotSubHistF11("RetC", aRetC, RetC0, dRetC, iRetC, nRetC)
ulalume3@0 1759 if (nTP > 0): PlotSubHistF11("TP", aTP, TP0, dTP, iTP, nTP)
ulalume3@0 1760 if (nTS > 0): PlotSubHistF11("TS", aTS, TS0, dTS, iTS, nTS)
ulalume3@0 1761 if (nRP > 0): PlotSubHistF11("RP", aRP, RP0, dRP, iRP, nRP)
ulalume3@0 1762 if (nRS > 0): PlotSubHistF11("RS", aRS, RS0, dRS, iRS, nRS)
ulalume3@0 1763 if (nRetT > 0): PlotSubHistF11("RetT", aRetT, RetT0, dRetT, iRetT, nRetT)
ulalume3@0 1764 if (nRetR > 0): PlotSubHistF11("RetR", aRetR, RetR0, dRetR, iRetR, nRetR)
ulalume3@0 1765 if (nERaT > 0): PlotSubHistF11("ERaT", aERaT, ERaT0, dERaT, iERaT, nERaT)
ulalume3@0 1766 if (nERaR > 0): PlotSubHistF11("ERaR", aERaR, ERaR0, dERaR, iERaR, nERaR)
ulalume3@0 1767 if (nRotaT > 0): PlotSubHistF11("RotaT", aRotaT, RotaT0, dRotaT, iRotaT, nRotaT)
ulalume3@0 1768 if (nRotaR > 0): PlotSubHistF11("RotaR", aRotaR, RotaR0, dRotaR, iRotaR, nRotaR)
ulalume3@0 1769 if (nLDRCal > 0): PlotSubHistF11("LDRCal", aLDRCal, LDRCal0, dLDRCal, iLDRCal, nLDRCal)
ulalume3@0 1770
ulalume3@0 1771 plt.show()
ulalume3@0 1772 plt.close
ulalume3@0 1773 '''
ulalume3@0 1774 # only histogram
ulalume3@0 1775 #print("******************* " + aVar + " *******************")
ulalume3@0 1776 fig, ax = plt.subplots(nrows=5, ncols=2, sharex=True, sharey=True, figsize=(10, 10))
ulalume3@0 1777 iLDR = -1
ulalume3@0 1778 for LDRTrue in LDRrange:
ulalume3@0 1779 iLDR = iLDR + 1
ulalume3@0 1780 LDRmin[iLDR] = np.min(aA[iLDR,:])
ulalume3@0 1781 LDRmax[iLDR] = np.max(aA[iLDR,:])
ulalume3@0 1782 Rmin = np.min(aA[iLDR,:]) * 0.999
ulalume3@0 1783 Rmax = np.max(aA[iLDR,:]) * 1.001
ulalume3@0 1784 plt.subplot(5,2,iLDR+1)
ulalume3@0 1785 (n, bins, patches) = plt.hist(aA[iLDR,:],
ulalume3@0 1786 range=[Rmin, Rmax],
ulalume3@0 1787 bins=200, log=False, alpha=0.2, normed=False, color = '0.5', histtype='stepfilled')
ulalume3@0 1788 plt.tick_params(axis='both', labelsize=9)
ulalume3@0 1789 plt.plot([LDRTrue, LDRTrue], [0, np.max(n)], 'r-', lw=2)
ulalume3@0 1790 plt.show()
ulalume3@0 1791 plt.close
ulalume3@0 1792 '''
ulalume3@0 1793
ulalume3@0 1794 # --- Plot LDRmin, LDRmax
ulalume3@0 1795 fig2 = plt.figure()
ulalume3@0 1796 plt.plot(LDRrange,LDRmax-LDRrange, linewidth=2.0, color='b')
ulalume3@0 1797 plt.plot(LDRrange,LDRmin-LDRrange, linewidth=2.0, color='g')
ulalume3@0 1798
ulalume3@0 1799 plt.xlabel('LDRtrue', fontsize=18)
ulalume3@0 1800 plt.ylabel('LDRTrue-LDRmin, LDRTrue-LDRmax', fontsize=14)
ulalume3@0 1801 plt.title(LID + ' ' + str(Type[TypeC]) + ' ' + str(Loc[LocC]), fontsize=18)
ulalume3@0 1802 #plt.ylimit(-0.07, 0.07)
ulalume3@0 1803 plt.show()
ulalume3@0 1804 plt.close
ulalume3@0 1805
ulalume3@0 1806 # --- Save LDRmin, LDRmax to file
ulalume3@0 1807 # http://stackoverflow.com/questions/4675728/redirect-stdout-to-a-file-in-python
volker@14 1808 with open('output_files\LDR_min_max_' + LID + '.dat', 'w') as f:
ulalume3@0 1809 with redirect_stdout(f):
ulalume3@0 1810 print(LID)
ulalume3@0 1811 print("LDRtrue, LDRmin, LDRmax")
ulalume3@0 1812 for i in range(len(LDRrange)):
ulalume3@0 1813 print("{0:7.4f},{1:7.4f},{2:7.4f}".format(LDRrange[i], LDRmin[i], LDRmax[i]))
ulalume3@0 1814
ulalume3@0 1815 '''
ulalume3@0 1816 # --- Plot K over LDRCal
ulalume3@0 1817 fig3 = plt.figure()
ulalume3@0 1818 plt.plot(LDRCal0+aLDRCal*dLDRCal/nLDRCal,aX[4,:], linewidth=2.0, color='b')
ulalume3@0 1819
ulalume3@0 1820 plt.xlabel('LDRCal', fontsize=18)
ulalume3@0 1821 plt.ylabel('K', fontsize=14)
ulalume3@0 1822 plt.title(LID, fontsize=18)
ulalume3@0 1823 plt.show()
ulalume3@0 1824 plt.close
ulalume3@0 1825 '''
ulalume3@0 1826
ulalume3@0 1827 # Additional plot routines ======>
ulalume3@0 1828 '''
ulalume3@0 1829 #******************************************************************************
ulalume3@0 1830 # 1. Plot LDRcorrected - LDR(measured Icross/Iparallel)
ulalume3@0 1831 LDRa = np.arange(1.,100.)*0.005
ulalume3@0 1832 LDRCorra = np.arange(1.,100.)
ulalume3@0 1833 if Y == - 1.: LDRa = 1./LDRa
ulalume3@0 1834 LDRCorra = (1./Eta*LDRa*(GT+HT)-(GR+HR))/((GR-HR)-1./Eta*LDRa*(GT-HT))
ulalume3@0 1835 if Y == - 1.: LDRa = 1./LDRa
ulalume3@0 1836 #
ulalume3@0 1837 #fig = plt.figure()
ulalume3@0 1838 plt.plot(LDRa,LDRCorra-LDRa)
ulalume3@0 1839 plt.plot([0.,0.5],[0.,0.5])
ulalume3@0 1840 plt.suptitle('LDRcorrected - LDR(measured Icross/Iparallel)', fontsize=16)
ulalume3@0 1841 plt.xlabel('LDR', fontsize=18)
ulalume3@0 1842 plt.ylabel('LDRCorr - LDR', fontsize=16)
ulalume3@0 1843 #plt.savefig('test.png')
ulalume3@0 1844 #
ulalume3@0 1845 '''
ulalume3@0 1846 '''
ulalume3@0 1847 #******************************************************************************
ulalume3@0 1848 # 2. Plot LDRsim (simulated measurements without corrections = Icross/Iparallel) over LDRtrue
ulalume3@0 1849 LDRa = np.arange(1.,100.)*0.005
ulalume3@0 1850 LDRsima = np.arange(1.,100.)
ulalume3@0 1851
ulalume3@0 1852 atruea = (1.-LDRa)/(1+LDRa)
ulalume3@0 1853 Ita = TiT*TiO*IinL*(GT+atruea*HT)
ulalume3@0 1854 Ira = TiR*TiO*IinL*(GR+atruea*HR)
ulalume3@0 1855 LDRsima = Ira/Ita # simulated uncorrected LDR with Y from input file
ulalume3@0 1856 if Y == -1.: LDRsima = 1./LDRsima
ulalume3@0 1857 #
ulalume3@0 1858 #fig = plt.figure()
ulalume3@0 1859 plt.plot(LDRa,LDRsima)
ulalume3@0 1860 plt.plot([0.,0.5],[0.,0.5])
ulalume3@0 1861 plt.suptitle('LDRsim (simulated measurements without corrections = Icross/Iparallel) over LDRtrue', fontsize=10)
ulalume3@0 1862 plt.xlabel('LDRtrue', fontsize=18)
ulalume3@0 1863 plt.ylabel('LDRsim', fontsize=16)
ulalume3@0 1864 #plt.savefig('test.png')
ulalume3@0 1865 #
ulalume3@0 1866 '''

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